The galaxy presents as a moderately sized, somewhat disturbed system. It shows a generally elliptical morphology, although with noticeable deviations from a perfectly smooth profile. There are indications of a central bulge, with the overall luminosity appearing brightest there, decreasing outwards. Faint, diffuse arms appear to extend from the central region, exhibiting a slightly disturbed structure. There is a suggestion of tidal features or minor interactions, possibly indicative of a past or ongoing merger event. The color profile suggests a mix of stellar populations; the core seems to have older stars while the outer regions may contain younger, bluer stars due to some recent star formation events, possibly induced by the interaction. Overall the image indicates a galaxy undergoing gravitational interaction.
