The galaxy presents a generally smooth and rounded morphology. There is little indication of significant disk structure or spiral arms. The light is concentrated towards the center, with a gradual falloff in intensity towards the outer edges. The galaxy's color appears yellowish-orange, indicating a stellar population dominated by older stars. There is no visible evidence of active star formation regions such as blue knots or HII regions. The overall appearance suggests an elliptical or lenticular galaxy, potentially at a considerable distance based on the lack of detailed features. No signs of ongoing merger activity or tidal disturbances are apparent within the observable field.
