The galaxy presents as an elongated structure, its morphology suggesting a possible elliptical or lenticular classification, though the resolution limits definitive categorization. There appears to be a central concentration of light, potentially indicating a galactic bulge. A subtle gradient in color is observed, transitioning from a slightly redder hue toward the core to bluer tones in the outer regions. This color gradient might imply differences in stellar populations, with older, redder stars concentrated centrally and younger, bluer stars populating the disk. There is a hint of asymmetry or minor disturbances in the outer region, although it is difficult to resolve any clear signs of a major merger event. The galaxy appears relatively isolated, though the low resolution makes it impossible to say if it has any companion galaxies. The absence of clearly defined spiral arms or significant dust lanes supports a classification leaning toward an early-type galaxy.
