The galaxy presents as a centrally concentrated, moderately luminous object, with an elliptical morphology. The core exhibits a bright, yellowish hue, suggestive of an older stellar population likely dominated by red giant stars. Moving outwards from the core, the color transitions to a more greenish-blue tone in some regions, possibly indicating some degree of ongoing or recent star formation. The galaxy appears relatively smooth and featureless, without any obvious spiral arm structure or strong dust lanes. A slight asymmetry is observable in the outer regions. There appears to be a minor disturbance in the structure; there might be a small companion galaxy or the remnants of a minor merger event. Overall, the galaxy appears to be an intermediate mass system.
