The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth and centrally concentrated light distribution. The primary body of the galaxy appears largely featureless. The light distribution suggests a moderate degree of roundness, tending more towards elliptical than perfectly spherical, yet not significantly elongated. There is a distinct secondary object extending from the bottom of the main galaxy. This secondary object exhibits a less concentrated light profile and a bluer hue. The galaxy does not appear to be undergoing any major merging events, although there is potentially evidence of a minor interaction occurring. Based on the overall color profile, the galaxy is likely a region with a redder hue.