The galaxy appears as a centrally concentrated, elliptical-like object with a smooth, diffuse profile. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outward from the center, the light gradually fades into a less intense, more reddish color, with the edges of the galaxy being poorly defined, blending into the background sky. There are no clear signs of spiral arms, bars, or significant dust lanes. It has a generally rounded shape, with only a very slight elongation. There is no visible evidence of recent or ongoing major merger activity or significant tidal disturbances. The overall appearance is consistent with a galaxy dominated by an older stellar population with relatively low levels of star formation.
