The galaxy appears as a relatively compact, centrally concentrated object. It exhibits a generally smooth morphology, although there may be subtle irregularities or distortions in its outer regions.

The light distribution suggests the presence of an extended halo or envelope surrounding a brighter, more concentrated core. There is a hint of asymmetry in the shape. The color profile exhibits a subtle variation, with the core potentially having a slightly bluer hue compared to the outer regions. The overall appearance is consistent with an elliptical galaxy or a lenticular galaxy viewed at a shallow inclination.

Based on visual inspection, there is no clear evidence of ongoing major mergers, although minor tidal interactions cannot be ruled out. Further analysis may be necessary to confirm or deny these features.
