The galaxy presents as a relatively compact object with a smooth, elliptical morphology. It exhibits a dominant central bulge, appearing almost spheroidal in shape. The light is concentrated towards the core. The light is yellowish. Based on the color profile, star formation is likely subdued, with a population of older stars dominating the emission. There is no clear evidence of spiral arms or dust lanes. The galaxy does not show any obvious signs of major mergers or tidal disturbances. However, there is a slight possibility of a minor disturbance based on irregular features.
