The galaxy presents as a somewhat elongated, lenticular-like object. It exhibits a smooth, diffuse morphology with no distinct spiral arm structure apparent. There is a central concentration of luminosity, suggesting a possible galactic bulge. The overall color appears to be relatively uniform throughout, leaning towards a slightly yellowish-green hue. This color profile implies a stellar population dominated by older stars, suggesting minimal ongoing star formation. There may be some evidence of minor tidal disturbance in the surrounding area. The overall shape is slightly elongated, hinting at a possible prolate spheroid. The galaxy does not appear to be actively merging or undergoing major interactions with any other visible galactic structures.
