The galaxy presents a generally smooth morphology, exhibiting a centrally concentrated luminosity profile. There is a slight elongation, but the overall shape appears relatively round, without any clear bar or spiral arm structures visible. Color gradients are subtle, with the central region displaying a slightly yellowish hue, suggestive of an older stellar population and diminished star formation activity. The outer regions appear somewhat bluer, hinting at the presence of younger, hotter stars, however, this blue color is very minimal. There is no evidence of significant tidal disturbances or ongoing mergers. The galaxy appears to be relatively isolated within its immediate environment. It presents itself as a relatively undisturbed system at intermediate redshift.
