The galaxy presents an overall elliptical morphology, appearing somewhat smooth in texture. There are no prominent spiral arms or a well-defined disk structure immediately apparent. The galaxy's light is concentrated towards the center, where a bright central bulge is evident. This bulge exhibits a yellowish-white hue, indicative of an older stellar population.

Extending outwards from the bulge, a fainter, less defined halo of light is observed. This halo appears less uniform and exhibits some irregularities, possibly suggestive of tidal interactions. The galaxy's color appears to shift towards a redder hue, suggesting ongoing star formation. There is also a slight blue hue visible in the bottom left of the halo.

A possible, but not entirely certain, minor disturbance is observable on the other side of the halo, indicating that this system may be in a late stage of galaxy merging.
