The galaxy presents as a moderately luminous object with a generally smooth, elliptical morphology. The central region exhibits a concentrated brightness, suggesting a significant stellar population density and potentially an active galactic nucleus, though the resolution is insufficient to confirm its presence. The isophotes appear mostly round, with a slight deviation towards an intermediate elliptical shape. There is little evidence of spiral arm structure or significant dust lanes. The colour profile indicates a redder core transitioning to a bluer halo, implying an older stellar population in the center and possibly more recent star formation in the outer regions. There is no readily apparent sign of any major mergers or significant tidal disturbances affecting the galaxy's overall form.
