The galaxy appears to be elliptical in shape, with a smooth, diffuse structure and a bright central bulge. It appears somewhat elongated, displaying a cigar-like morphology rather than perfectly round. The color gradient suggests that the core regions are yellower and the outer areas are slightly redder. The overall color seems to indicate an older stellar population. There is no discernible spiral arm structure nor evidence of any ongoing major merger events. The galaxy appears isolated and unperturbed.
