The galaxy presents as a relatively smooth, centrally concentrated object. The morphology is generally elliptical or lenticular, showing a lack of prominent spiral arms or a distinct disk structure. The light is dominated by warmer colors, suggesting an older stellar population with limited ongoing star formation. There is some asymmetry present, and the galaxy shows evidence of a possible tidal tail or disturbance to the lower part of the main body. The central region appears bright and somewhat unresolved. The galaxy could be undergoing or have recently undergone a minor merger event.
