The galaxy presents as a disk-shaped structure, viewed at a moderately inclined angle. Its overall morphology appears relatively smooth, with a concentrated central bulge exhibiting a bright, high-luminosity core, indicative of a significant stellar population density. The disk component displays a subtle color gradient, with a bluer hue towards the outer regions suggesting ongoing star formation, in contrast to the yellower, more evolved stellar population concentrated in the central bulge. There is a subtle hint of asymmetry in the outer disk structure, possibly suggestive of tidal interactions, minor disturbances, or a lopsided distribution of stellar material within the disk. There is no obvious presence of defined spiral arms or prominent dust lanes.
