The galaxy presents as a relatively compact object, characterized by a notable concentration of light in its central region. The morphology appears to be smooth overall, with a centrally concentrated bulge that constitutes the majority of the galaxy's visible structure. There are hints of features that could suggest tidal interactions or disturbances; this is supported by the presence of a secondary, somewhat ambiguous source or distortion near its main body, giving the appearance of an ongoing or recent merger event. There is a lack of prominent spiral arm structures, giving the impression of an elliptical or lenticular galaxy undergoing some form of interaction. The color of the galaxy appears redder, indicating the presence of an older stellar population. A relatively low rate of star formation is inferred.
