The galaxy presents as a relatively well-defined, centralized object with a generally smooth morphology. The primary component exhibits a concentrated, rounded appearance with a slight elongation suggestive of an elliptical or lenticular form. There's a subtle indication of possible disturbances or minor features, but the light distribution appears largely uniform.

Color analysis suggests a population of older stars, exhibiting a reddish hue throughout the majority of the structure, potentially signifying the presence of a more evolved stellar population. There is some very subtle variation in color across the galaxy, but this is not a strong feature. Overall, the galaxy appears relatively quiescent in terms of star formation. Indications of merging or major disturbances are not strongly apparent.
