The galaxy appears as an elliptical or lenticular-type, showing a generally smooth light distribution. The primary body has a concentrated, centrally bright core that diffuses outwards. There is a smaller body in close proximity, possibly a dwarf galaxy, showing a somewhat similar but less concentrated luminosity. Its proximity suggests a possible interaction, though no clear tidal features or distortions are readily apparent in the main galaxy's structure. The color profile is skewed towards the redder end of the spectrum, particularly within the central region, indicative of a more evolved stellar population.
