The galaxy appears as a relatively compact and elliptical-shaped structure. The central region exhibits a bright, yellowish hue, indicative of an older stellar population. A lack of prominent spiral arms or dust lanes suggests it is a relatively smooth galaxy, potentially an elliptical galaxy.

There is an object that appears to be a disturbed spiral galaxy close by and potentially interacting.

The overall color profile suggests a galaxy with limited ongoing star formation and a dominant population of older, redder stars. The galaxy appears to be relatively isolated, although I cannot rule out minor tidal interactions.
