The galaxy presents as an elongated, cigar-shaped structure, with a significantly higher probability of being cigar shaped than round. It does not present any roundness. The galaxy displays a notable central bulge that appears to be a relatively smooth, homogenous region, transitioning into the outer regions. There is some indication of disk-like features, although they are not sharply defined and may be part of a more diffuse structure. The color profile suggests a mix of stellar populations. The central region shows a yellowish to whitish hue, which could indicate an older stellar population. There are hints of bluer, possibly younger stars in the outer disk regions, but the overall blue component is moderate. There are no obvious signs of recent major merger events. The main body of the galaxy is intact. There may be minor disturbances or tidal features, potentially suggestive of past interactions or accretion events.
