The galaxy presents as a relatively luminous and compact system with an apparent smooth morphology. There are no easily discernible spiral arms or a central bar feature. The galaxy's light profile appears concentrated, with a moderately bright core region that fades into a more diffuse halo. The overall color appears to be on the redder end of the spectrum, suggesting an older stellar population and/or significant dust obscuration. There is an indication of possible gravitational interaction or tidal disturbance, with a slightly irregular shape. A secondary, less prominent concentration of light is visible along the halo, possibly indicative of a minor merger event. Overall, the galaxy appears to be a passively evolving system that is in the process of merging or has recently undergone a merger event.
