The galaxy appears as a centrally concentrated object with a fairly smooth light distribution. It exhibits an elliptical morphology, appearing mostly round with a very slight elongation. The core of the galaxy shows a bright, compact nucleus, surrounded by a more diffuse halo of light. The color profile suggests a dominant population of older stars, with a redder hue in the central regions and a slightly bluer tint towards the outer edges of the halo, potentially indicating some ongoing star formation. There are no obvious spiral arms or bar features visible, and the galaxy appears relatively undisturbed, lacking significant signs of recent or ongoing mergers or tidal interactions.
