The galaxy presents as a centrally concentrated, elliptical morphology. The light profile is smooth and lacks distinct spiral arm structures or prominent dust lanes. It has a moderate ellipticity, being more oblong than perfectly circular, and shows a gradual decrease in brightness moving outward from the nucleus. The core appears bright and yellow, suggesting an older stellar population. There is no clear evidence of ongoing major mergers or tidal disturbances. The galaxy appears relatively isolated within the observed field. Overall, the galaxy appears as a massive, quiescent system dominated by evolved stars.
