The galaxy presents as an elliptical morphology, elongated in shape. The core exhibits a bright, concentrated luminosity gradient, appearing yellowish, suggesting an older stellar population and potentially a significant dust content. Progressing outward from the core, the color transitions toward a bluer hue, possibly indicating the presence of younger stars or a less obscured view through the galaxy's outer regions. The galaxy appears relatively smooth in texture with no visually distinct spiral arm structures or prominent dust lanes visible within the limits of this image resolution. There are no indications of tidal tails, or other major mergers. The overall structure suggests a galaxy that is in a relatively quiescent state regarding major merger events.