The galaxy appears to be an elliptical galaxy. It exhibits a smooth, diffuse light profile, increasing in intensity towards the center. The galaxy shows a slightly elongated shape, with a ratio of approximately 2:1 between its major and minor axes. There is no evidence of spiral arms or a prominent disk structure. The color suggests an older stellar population, with a yellow-red hue dominating. There is very little blue light visible. The morphology implies that any recent or ongoing star formation activity is minimal, the bulk of the galaxy's mass is likely in older stars. There is no strong evidence of any merging activity or tidal disturbances affecting its shape, though this could be subtle.
