The galaxy presents an elliptical morphology, appearing as a flattened spheroid with a noticeable bulge. Its overall color profile leans towards a redder hue, suggesting a population of older stars. There seems to be a smooth, gradual decline in luminosity from the core outwards. The galaxy exhibits a degree of asymmetry in its light distribution and the isophotes appear slightly twisted. The image suggests a galaxy that may be either an isolated elliptical or undergoing some form of interaction or recent disturbance, evidenced by the slight morphological peculiarities. There is a companion galaxy nearby, which may have caused the disturbances. There are no spiral arms visible.
