The galaxy presents as an elongated, cigar-shaped structure, indicating a likely elliptical morphology or potentially a highly inclined spiral galaxy. The central region exhibits a yellow-orange hue, suggestive of an older stellar population, potentially a bulge dominated by evolved stars. Moving outward from the core, the color transitions to a bluer tone, hinting at the presence of younger, hotter stars in the outer regions. The galaxy appears relatively smooth in texture, with no prominent dust lanes or spiral arm structures visible. There is a subtle asymmetry in the outer regions, possibly due to tidal interactions or minor disturbances. No clear evidence of ongoing major merger activity is readily apparent, though subtle distortions suggest a potential for past or ongoing minor interactions. The size of the galaxy appears to be considerable, indicating a potentially massive system. Overall, the galaxy appears to be a luminous, moderately evolved system with some hints of disturbance in its past.
