The galaxy presents a generally smooth morphology, appearing elongated in shape. The light profile appears to be centrally concentrated, indicative of a substantial bulge component. The galaxy exhibits a color gradient, transitioning from a bluer hue in the outer regions to a redder, more yellowish hue towards the center. This suggests a potential gradient in stellar populations, with younger, bluer stars dominating the outskirts and older, redder stars concentrated within the bulge. There appears to be little to no indication of well-defined spiral arm structures or dust lanes. There is a faint red spot slightly away from the central area, but generally the galaxy shows no signs of active merging or significant tidal disturbances.
