The galaxy appears as a centrally concentrated, elliptical-like object. It exhibits a smooth and somewhat diffuse morphology with a fairly uniform light distribution. The core is bright, with the luminosity gradually decreasing toward the outer regions. No distinct spiral arms, bars, or prominent dust lanes are discernible. The galaxy seems to be relatively isolated, with no obvious signs of tidal interactions or major mergers affecting its structure. Based on its color, which presents as a warm yellow, the stellar population is likely older on average, with relatively low ongoing star formation.
