This galaxy appears to be an elliptical galaxy with a generally smooth morphology. The galaxy exhibits a central bulge that appears significantly brighter than its surrounding components. The overall shape is elongated, with the major axis more extended than the minor axis. The light distribution is centrally concentrated, with the intensity decreasing gradually towards the outer regions. There is a subtle color gradient, with the central bulge appearing yellower, possibly indicating a population of older stars. Fainter, bluer components are observed on the edges. These could possibly be spiral arms, indicating a spiral structure. This observation requires higher resolution imaging for verification. The galaxy seems relatively undisturbed, showing no obvious signs of recent merger activity or tidal interactions. The galaxy is inclined with respect to our line of sight.
