The galaxy presents as a somewhat elliptical shape with a fairly smooth morphology, yet displaying some disturbances. The central region exhibits a concentrated luminosity suggesting the presence of a bulge, likely containing older stellar populations. Fainter, diffuse light extends outwards from the central bulge, giving the galaxy an overall fuzzy appearance. The overall color profile leans towards the redder end of the spectrum, potentially indicating a relatively quiescent galaxy with a lower rate of current star formation, and a dominance of evolved stars. Despite the relatively smooth appearance, there are possible signs of minor tidal disruptions. The disk, if present, is not clearly defined, and the galaxy does not appear to be undergoing a major merger event, but minor interactions cannot be ruled out. The galaxy is estimated to be of significant mass, given its brightness at a redshift of approximately 0.22.
