The galaxy presents as a somewhat elongated structure with a noticeable central bulge. The color profile suggests an older stellar population, with reddish hues dominating the core region. There is some indication of a slight disk-like component, although it is not well-defined, possibly due to the galaxy's overall shape or viewing angle. The morphological classification leans towards a smooth structure, yet there is an asymmetry that indicates a possible interaction or disturbance. No clear spiral arms or intense star-forming regions are apparent in this image. The galaxy is relatively compact, with a diffuse outer halo extending from the central region. Overall, the galaxy appears to be an evolved system, potentially an elliptical or lenticular galaxy that has undergone some form of gravitational interaction in its past.
