The galaxy appears as a centrally concentrated, elliptical-like structure. It exhibits a smooth, featureless morphology with a dominant bulge component and a diffuse halo. There's a clear color gradient visible, trending from a yellowish core to a slightly redder outer region. This suggests an older stellar population is concentrated in the center, with potentially younger stars distributed throughout the halo. The galaxy presents an overall moderate to high luminosity. No clear signs of significant ongoing star formation are immediately apparent from the image, nor are there any major signs of interaction or tidal disturbances. It does not appear to be undergoing a major merger. There appears to be a minor disturbance or perhaps a small merger happening. The galaxy possesses a noticeable degree of roundness, deviating somewhat from a perfectly elliptical shape, though it is not highly elongated.
