The galaxy presents as a relatively smooth, disk-dominated structure. The central bulge is prominent and exhibits a concentrated luminosity, suggesting a high density of stars. Moving outwards from the bulge, a flattened disk is observable, although the resolution limits detailed morphological classification. The disk exhibits a color gradient, transitioning from a more yellow/orange hue near the central bulge to a slightly bluer tint in the outer regions. This suggests a difference in stellar populations, with older, redder stars concentrated in the bulge and younger, bluer stars populating the disk. The overall form is not perfectly symmetrical; there appears to be some minor disturbance or irregularity in the disk structure, potentially indicating past or ongoing interactions. No strong evidence of a recent major merger event is visually apparent. Star formation seems to be occurring in a relatively restrained manner, without significant, bright HII regions or intense blue clusters easily discernable in the disk. The galaxy's light output is quite substantial, implying a large stellar mass.
