The galaxy presents a predominantly smooth and rounded morphology. A central bulge is readily apparent, exhibiting a concentrated luminosity profile that declines towards the outer regions. The overall color index suggests the presence of an older stellar population, with a relative deficiency in blue light. There is a subtle indication of a disk component that is either heavily obscured or intrinsically faint. There is an indication of minor disturbances, with some slight asymmetrical features. There is no evidence of spiral arm structure or significant dust lanes. 