The galaxy presents as an elongated, elliptical form with a distinct central bulge exhibiting a concentrated luminosity. The overall color profile leans towards warmer tones, suggesting a stellar population dominated by older, redder stars, particularly within the bulge region. Fainter, bluer hues are observed peripherally, hinting at the presence of younger, hotter stars. The galaxy appears relatively smooth and undisturbed, with no obvious signs of recent major mergers or significant tidal interactions. The shape deviates from a perfect circle, appearing more cigar-shaped than round. There is little evidence of prominent spiral arms or a well-defined disk structure. The system has no visible bar structure. Overall, the galaxy presents characteristics consistent with an elliptical galaxy with a moderate mass.
