The galaxy appears as a single, luminous object, exhibiting a generally elliptical morphology. The light distribution is concentrated towards the center, suggesting a prominent galactic nucleus. The object displays a smooth appearance, with no readily discernible spiral arms or complex structures typically associated with actively star-forming galaxies.

The galaxy exhibits a yellowish-red hue, possibly indicative of an older stellar population and a relatively low rate of on-going star formation. There is a smaller yellowish companion galaxy in close proximity, suggesting a potential gravitational interaction or merger event may be occurring. Faint, reddish diffuse emission extends from the main body of the galaxy, which may be tidal debris or evidence of past activity. There may be a tidal tail present as well. Overall, the galaxy appears to be a relatively evolved system, with a high degree of central concentration and a quiescent star formation history.
