The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a concentrated luminosity with a yellowish hue, suggesting an older stellar population. The outer regions display a less concentrated and somewhat diffuse light distribution that is tinged with blue. There is no clear presence of spiral arms or a distinct disk-like structure. The overall shape is generally rounded. There's no evidence of any major disturbances or ongoing merging activity, although subtle irregularities in the outer regions might hint at minor gravitational interactions. The galaxy appears to be relatively isolated in the image.
