The galaxy presents as a single, relatively compact object. It exhibits a centrally concentrated luminosity profile, appearing brightest at its core and gradually fading outwards. The overall morphology is predominantly smooth, suggesting an elliptical classification or potentially a spiral galaxy viewed face-on without prominent spiral arms. The shape is neither perfectly circular nor elongated; it presents with an intermediate ellipticity. There is a subtle hint of a possible minor disturbance or asymmetry in the outer regions, but it is not a clear indication of a major merging event. The primary color of the galaxy appears to be a slightly reddish hue. This may indicate an older stellar population. 
