The galaxy presents as an elliptical morphology, appearing largely smooth and centrally concentrated with a high degree of symmetry. It has a discernible, extended halo of diffuse light. The core region exhibits a yellowish hue, potentially indicative of an older stellar population. A fainter secondary structure, offset from the primary body, displays a reddish tone. This feature could be the result of a tidal interaction with the main galaxy, or a smaller galaxy in the process of merging. No spiral arm structures are observed. Based on its color and shape, it appears to be a massive galaxy with low star formation. The galaxy's color profile suggests relatively low specific star formation rate. The absence of dust lanes or prominent features typical of active star formation supports this assessment.