The galaxy exhibits a generally smooth, elliptical morphology. It appears quite round with a very minor elongation. There is little visible internal structure, no obvious spiral arms, and no indications of a bar feature. The central region exhibits a slight concentration of light, but it's not particularly pronounced, suggesting a relatively diffuse core. The galaxy appears relatively isolated, with no clear signs of major tidal interactions or mergers with nearby objects. There might be a slight distortion in the galaxy's outer isophotes, suggesting minor past interactions, though these are not definitive. The galaxy has a redder color, indicative of a relatively older stellar population and a low rate of star formation, as well as a high mass.
