The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology. Its shape is elongated, resembling a cigar, with a high degree of axial ratio. The light distribution is centrally concentrated, with the brightest region located at the core. There is a color gradient, with the core exhibiting a yellowish hue, possibly indicative of an older stellar population. The outer regions appear fainter with a slight shift towards redder colors, further suggesting an aging stellar population. There is no visible evidence of spiral arms, dust lanes, or recent star formation activity. The galaxy does not appear to be undergoing any major mergers or interactions, appearing relatively undisturbed.
