This galaxy exhibits a dominant, smooth bulge component, appearing largely spheroidal in shape. The central region displays a concentrated luminosity, indicating a possible active galactic nucleus or a dense stellar population. Faint, diffuse extensions emanate from the core, hinting at a disrupted disk or tidal features resulting from past interactions. The overall color profile suggests a population of older stars, but there are hints of more recent star formation regions, possibly in the outer regions. There is evidence of interaction with another nearby galaxy; a potential minor disturbance of the disk is present.
