The galaxy presents as a relatively smooth, elliptical-like structure. The central region displays a concentrated luminosity with a yellow-orange hue, indicative of an older stellar population. Moving outward from the core, the color gradually shifts towards a bluish tint, potentially suggesting the presence of younger, hotter stars or ongoing star formation regions. The galaxy appears to be moderately extended, but without a clearly defined disk structure or prominent spiral arms. There are some subtle irregularities in the outer regions that indicate some kind of minor disturbance.
