The galaxy presents as a single, relatively smooth, and rounded entity. It exhibits a concentrated central region that appears to be spheroidal in shape. The core displays a yellowish hue, suggesting an older stellar population dominating the emission. Moving outward from the core, the color transitions subtly towards redder tones, possibly indicating the presence of dust or cooler stars in the outer regions. The outer regions of the galaxy appear diffuse, with no distinct spiral arm structures or prominent features visible. There are no obvious signs of tidal disturbances or ongoing major merger events. The overall morphology suggests the classification as an elliptical galaxy.
