The galaxy presents as a concentrated, elliptical morphology with a smooth, featureless appearance. It exhibits a predominantly yellow-orange hue, suggesting a population of older stars and potentially lower levels of ongoing star formation. The central region is notably brighter, indicating a higher density of stellar mass concentrated toward the core. There is a small, dimmer region to the left and bottom of the galaxy core which could be either be part of the galaxy, or a separate object behind or in front of the galaxy in question. The galaxy appears relatively undisturbed, with no obvious signs of tidal interactions or major mergers.
