The galaxy presents as a single, centrally concentrated object with a generally smooth, elliptical morphology. There's a slight elongation, but it is mostly round in appearance. The luminosity appears highest in the central region, decreasing smoothly outwards, suggesting a lack of spiral arm structures or significant dust lanes. The color profile indicates a yellow-red hue, possibly signifying an older stellar population. There is no evidence of ongoing major mergers or tidal disturbances in the immediate vicinity of the galaxy.
