The galaxy appears as a relatively smooth, centrally concentrated object with a generally elliptical morphology. There is a notable lack of distinct spiral arms or a bar structure. The light distribution suggests a high degree of central symmetry. The galaxy exhibits a somewhat diffuse halo, gradually fading into the background sky, with no evidence of ongoing major merging events or significant tidal disturbances. Color gradients are subtle but present, with the central region appearing slightly bluer compared to the outer regions, which trend towards redder hues. Overall, the galaxy presents as a well-formed, undisturbed system.
