The galaxy presents as a single, resolved object exhibiting both smooth and featured characteristics. It appears to be an elliptical galaxy undergoing a possible merger.

The central region displays a concentrated, bright, and yellowish core, indicating a significant population of older stars. The radial profile around the core shows a relatively smooth distribution of light.

A fainter, bluer, and more diffuse structure is observed on the left side of the galaxy. This feature suggests a separate component interacting with the primary galaxy body. There is evidence of tidal distortion in the form of slight asymmetry and extended diffuse light suggesting minor gravitational disturbances, perhaps indicative of an ongoing or recent interaction.

The overall shape is neither perfectly round nor highly elongated but presents a compromise.

The presence of both smooth, older stellar populations and bluer, potentially younger features indicates a complex star formation history possibly influenced by the interaction.
