The galaxy presents as a flattened elliptical morphology, approximately 4.5 kpc in radius based on light distribution. The central region exhibits a yellow hue, suggestive of an older stellar population. There is some bluer emission on the edges, suggesting areas of recent star formation. Some asymmetry in shape indicates a mild level of tidal disturbance, though not a major ongoing merger. The overall structure is dominated by a smooth component; signs of spiral arms are absent. The galaxy appears to be generally isolated, and no obvious companion galaxies are interacting.