The galaxy presents a generally smooth morphology, suggesting it is an elliptical galaxy. It has a concentrated, round central region that dominates the visual appearance, with a gradual decrease in brightness towards its outer edges. There are slight hints of diffuse features or a very faint disk structure but these are indistinct. There do not appear to be prominent spiral arms or significant dust lanes visible, nor does there seem to be any tidal disturbance or evidence of merging activity. Its color appears to be trending towards the redder part of the spectrum. This would imply a galaxy dominated by an older stellar population.
