The galaxy appears to be an elliptical or lenticular galaxy, with a smooth, featureless profile. It shows a slight elongation, but not a distinct spiral structure. The core is bright and concentrated, indicative of an older stellar population, with a general redder overall color. There is no evidence of a major ongoing merger, but subtle irregularities suggest possible past minor interactions. The galaxy appears well-defined against the background sky, with a moderate size.
