The galaxy presents a relatively smooth morphology, suggesting an elliptical or lenticular type. It exhibits a notable central bulge that appears to be moderately elongated, almost cigar-shaped. A faint, diffuse halo surrounds the central structure, with a greenish hue, indicating the presence of ionized gas and potentially recent or ongoing low-level star formation. The color distribution within the galaxy indicates a complex stellar population, with bluer components in the central region, possibly representing younger stars, and a general reddening towards the outer regions, consistent with an older stellar population. There are no prominent spiral arms or other features indicative of a classical spiral galaxy, and no apparent signs of active galactic nuclei or significant dust lanes. There may be a minor tidal interaction occurring, indicated by some slight distortion in the overall shape and an asymmetric halo.
