The galaxy presents as a somewhat smooth, elliptical structure. The central bulge is prominent and exhibits a reddish-orange hue, suggesting an older stellar population dominated by redder giants and dwarfs. The light emanating from the central region is more concentrated, indicating a higher stellar density.

Moving outwards from the core, the color transitions to a greenish-blue, indicative of younger, hotter stars and possibly some ongoing star formation. This outer region appears less structured and more diffuse than the central bulge, implying a lower stellar density.

There are no obvious signs of a spiral arm structure. No significant tidal tails or distorted features are visible, suggesting that this galaxy has not undergone any major merging events recently. The galaxy’s overall shape appears close to being round. There are no apparent signs of significant dust lanes obscuring any part of the galaxy.
