The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The color profile indicates a dominant population of older stars, exhibiting a redder hue in the central region transitioning to slightly bluer tones in the outer disk. There is an indication of a possible minor disturbance, with a faint, diffuse object offset from the main galactic body, suggesting a potential tidal interaction or a dwarf galaxy companion. The galaxy appears relatively isolated. There is no strong evidence of active star formation within the galaxy.
