The galaxy presents a relatively smooth, elliptical morphology. It is centrally concentrated with a bright, yellowish core indicative of an older stellar population. The overall shape appears close to circular, with a slight deviation towards a more elongated form. There's little evidence of distinct spiral arms or significant dust lanes. The galaxy exhibits a gradual decrease in surface brightness moving outwards from the core, eventually fading into the background sky. No significant merging or tidal disturbances are visually apparent, suggesting a relatively isolated and stable system.
