The galaxy presents as a smooth, elliptical morphology. The light profile is centrally concentrated, with a gradual decrease in surface brightness towards the outer regions. There is an absence of distinct spiral arms or a prominent disk structure. The galaxy exhibits a yellowish hue, indicative of an older stellar population. The overall shape appears moderately flattened, with the major axis extending along a Northwest to Southeast orientation. There is a possibility of minor tidal disturbances, suggesting a potential history of interactions or mergers. The galaxy's Sersic index suggests a relatively high concentration of light in the central region. The color profile suggests the presence of dust, or a gradient in stellar populations.
