The galaxy presents as a relatively smooth, rounded object. It appears to be an elliptical galaxy, with minimal discernible features such as spiral arms or a prominent disk structure. The overall color profile suggests a dominant population of older stars, indicating a potentially lower rate of ongoing star formation. There are some regions of bluer emission, suggestive of younger stellar populations and some ongoing star formation. There is no clear evidence of a recent major merger or tidal disturbances. The galaxy appears to be relatively isolated.
