The galaxy presents as a somewhat inclined disk, suggesting a possible spiral or lenticular morphology. The central bulge appears relatively bright and concentrated, exhibiting a yellowish hue indicative of an older stellar population. The disk component shows a bluer color, which may signify more recent star formation. While the image resolution is limited, there is a subtle hint of spiral arm structure extending from the central bulge. The galaxy appears largely undisturbed, with no obvious signs of major mergers or tidal interactions. There may be some areas of dim dust lanes within the galaxy, although the low image quality makes it difficult to discern the structures in great detail. The overall color profile indicates a galaxy with a mix of stellar populations, with the central regions dominated by older, redder stars and the outer disk showing evidence of ongoing star formation.
