The galaxy appears to be a relatively compact, luminous object, showing an overall elliptical morphology. The light distribution seems smooth, with a centrally concentrated core. There is an extended halo of light surrounding the core that is noticeably distorted.

Within the extended halo, a secondary, smaller object is visible. The secondary component is similar in color to the primary component and appears to be tidally disrupted. This suggests a possible minor merger or tidal interaction.

The overall color of the system appears to be yellowish-white, suggestive of a stellar population with a mix of both old and intermediate age stars. The light emitted from the central portion of the galaxy appears to be slightly redder in color than light emitted by the tidal disturbance.
