The galaxy presents a relatively smooth, elliptical morphology. The light profile appears centrally concentrated with a gradual decrease in intensity towards the outer regions. There are no distinct spiral arms or other significant features suggestive of a disk component. The galaxy's color is generally red, implying a dominant population of older stars. A small fraction of blue light is noticeable, hinting at some ongoing, but likely subdued, star formation activity. No signs of major mergers are apparent, though there is possible evidence of minor gravitational interaction or disturbance. The galaxy's overall shape is close to circular with no significant elongation.
