The galaxy appears as a centrally concentrated object with a generally smooth morphology, displaying a somewhat elliptical shape. The core is brighter and yellowish. The galaxy exhibits a faint disk, which is difficult to discern. Its overall structure suggests an evolved system, potentially an early-type spiral or a lenticular galaxy approaching a more spheroidal form, with a stellar mass estimated to be approximately 10^10.8 solar masses. The star formation rate is relatively low, suggesting a population dominated by older stars. There is no visually apparent evidence of major mergers or significant tidal disturbances affecting the galaxy's morphology.
