The galaxy presents as a smooth, elliptical structure, with a noticeable concentration of light toward the center. The core region exhibits a bright, yellowish-white hue, indicative of an older stellar population. Moving outward from the core, the color gradually shifts towards a redder and fainter profile. There is a subtle asymmetry to the overall shape, but no clear evidence of spiral arms or prominent dust lanes. The galaxy appears relatively isolated with no obvious signs of ongoing mergers or tidal disturbances.
