The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge, with a gradual decrease in surface brightness moving outwards. The morphology is generally round, lacking any obvious strong tidal features or signs of major mergers. There are no significant spiral arm structures visible. The light distribution suggests an older stellar population, more concentrated towards the center, contributing to its yellow-reddish hue. The object does not show any signs of active star formation, except possibly within the central bulge region, as implied by its overall color profile. There are no strong indications of significant dust lanes or obscuration. The galaxy appears to be relatively isolated in its environment.
