The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a generally elliptical morphology, with a noticeable lack of distinct spiral arms or a bar structure. The light distribution is concentrated towards the core, which emits a bright, yellowish glow. This suggests a significant population of older stars. Fainter, less defined regions of color extend outwards, hinting at some low-level ongoing or recent star formation. There is no indication of significant tidal disturbances or merger activity in this image. The object presents as a fairly quiescent galaxy, possibly an early-type spiral or an elliptical galaxy.
