The galaxy appears as a relatively smooth, elongated structure. Its light distribution suggests a centrally concentrated bulge or core, with a gradual decrease in brightness towards the outer edges. The galaxy's overall color is somewhat neutral, indicating a mix of stellar populations. There isn't much evidence of distinct spiral arm structure or significant dust lanes. The morphology is consistent with an elliptical or lenticular galaxy, and the smooth light profile suggests that a large fraction of stars formed long ago. There appears to be no interaction with other large galaxies.
