The galaxy exhibits a relatively smooth morphology, with a high degree of central concentration. The light distribution appears roughly elliptical in shape, with a high degree of circularity. It is likely that this is an elliptical galaxy due to its smooth features and lack of spiral arms.

The color profile suggests a population dominated by older stars, with a yellowish hue concentrated towards the galactic center. A very faint blue color is seen at the edges of the object, suggesting a small number of younger, hotter stars at the edges of the object.

There are no obvious signs of significant tidal disturbances or ongoing major mergers. The galaxy appears to be relatively isolated and undisturbed.
