The galaxy presents as a somewhat elliptical, though not perfectly round, morphology. The central region exhibits a brighter, concentrated luminosity suggesting a prominent bulge. This region is primarily white in color, indicating a likely older stellar population. Fainter, bluer light emanates from what appears to be the disk component. This suggests the presence of ongoing star formation within the disk, albeit at a relatively low rate. The disk appears somewhat disturbed, hinting at a possible minor interaction or past merger event. Overall, this galaxy is likely a disk galaxy exhibiting features of an aging stellar population and relatively low star formation.
