The galaxy presents as a centrally concentrated, smooth, and rounded structure. The light profile suggests an elliptical morphology, with a notable absence of spiral arms or prominent disk features. The core of the galaxy exhibits a bright, yellowish hue, indicating a significant population of older stars. The galaxy appears to be relatively isolated, with no obvious signs of a major merger or tidal disruption. The overall appearance suggests a quiescent galaxy with a low star formation rate.
