The galaxy presents as an elliptical morphology, appearing largely smooth in structure. There is a slight elongation in the horizontal axis, suggesting a mild departure from a perfectly spherical shape. The central region is bright and concentrated, with the light gradually diminishing towards the outer edges. The color profile appears relatively uniform with a yellowish tint in the center, indicating a population of older stars and a lower rate of ongoing star formation. There is some slight bluing in the outer regions indicating some faint presence of younger stars. No spiral arms or dust lanes are readily apparent, reinforcing the classification as an elliptical type galaxy. There appears to be no major ongoing merger events or tidal disturbances visible in the immediate vicinity of the galaxy.
