The galaxy presents a generally smooth morphology, suggesting it is likely an elliptical or lenticular galaxy. There is some evidence of faint disk-like features or perhaps tidal disturbances, but the light distribution is primarily concentrated toward the center. The shape is somewhat elongated but not significantly so, with no clear cigar shape visible. The central region exhibits a yellowish-red hue, possibly indicating an older stellar population or the presence of dust obscuration. A small blue region is visible on the outer edge, potentially indicating an area of ongoing star formation. There are indications of some interactions or disturbances, although there is no clear indication of major merging activity. Overall, it is a relatively massive galaxy with moderate star formation activity.
