The galaxy presents as a moderately sized, lenticular or early-type spiral structure. Its overall form appears relatively smooth, with a subtle central bulge. A faint, diffuse disk is visible, though distinct spiral arms are not readily apparent in the provided image. The galaxy exhibits a slightly elongated shape, deviating somewhat from perfect circularity, with its longest side measuring just over 4 arcseconds, suggesting a classification between round and cigar-shaped. Evidence of minor disturbance or potential interactions exists, as hinted by slight asymmetries or irregularities in the disk's outer regions. Color gradients suggest the presence of an aging stellar population. There is a lack of prominent blue regions indicative of massive star formation and an overall redder color, which is typical of galaxies with low star formation rates.
