The galaxy appears as a concentrated, luminous spheroid. The primary color is a warm yellow-orange, suggesting a population of older stars and a relatively quiescent star formation rate. There is a slight color gradient, with the core appearing more yellow and the outer regions exhibiting a slightly redder hue, potentially indicating a radial difference in stellar populations or dust content. The galaxy's overall form is smooth and generally featureless with a subtle disk-like shape. There is no apparent evidence of spiral arms or other distinct structural details, nor any major disturbances or merging activity in progress. It appears to be a fairly relaxed system, with most of the light concentrated centrally.
