The galaxy presents an overall smooth morphology, with a shape that is somewhere between rounded and elongated, appearing somewhat cigar-shaped. There is a distinct central bulge region which is brighter and more concentrated, exhibiting a reddish hue. Surrounding the bulge, a fainter, bluish halo or disk-like structure is observed. There are no strong indications of spiral arms, bars, or significant dust lanes. The galaxy does not appear to be undergoing a major merger, although there may be evidence of a minor disturbance in its structure. The overall color suggests a population dominated by older stars, particularly in the central bulge, with perhaps a younger, bluer population contributing to the outer regions. Star formation is likely occurring at a relatively low rate.
