The galaxy presents as a relatively compact, elliptical morphology. Its light profile is generally smooth, lacking prominent spiral arms or a defined disk structure. The shape appears to be somewhat elongated, exhibiting a slight cigar-like appearance.

The galaxy's color gradient shows a central region that is slightly bluer than its outer edges. This color variation suggests the presence of a younger stellar population in the core, possibly indicating ongoing or recent star formation activity. Overall, the galaxy's luminosity suggests it is a massive system.

There are no obvious signs of major mergers or significant tidal disturbances. There may be a companion galaxy present nearby.
