The galaxy presents as a centrally concentrated, relatively smooth structure, likely an elliptical or lenticular galaxy given the absence of prominent spiral arms. The light is dominated by a yellowish hue at the core, indicating an older stellar population. A bluer halo surrounds the central bulge, suggesting the presence of a younger stellar population or ongoing star formation. The galaxy exhibits a slight degree of asymmetry, possibly indicative of a minor interaction or disturbance in its recent past. Faint, irregular features are observed extending outwards which could be tidal debris from a past interaction. The overall morphology leans towards a slightly elongated shape, though not definitively cigar-shaped. There's no strong evidence of a major merger or ongoing, significant disturbance.
