The galaxy presents an elliptical morphology, exhibiting a smooth, centralized concentration of light. It appears to be somewhat elongated in shape, deviating from a perfectly circular form. A color gradient is observed, with a yellowish hue dominating the central region, potentially indicating an older stellar population. Moving outward, the color shifts towards redder tones, which may suggest the presence of dust or a change in the stellar population distribution. No prominent spiral arms or distinct features such as star-forming regions are discernible. There are no obvious signs of major mergers or significant tidal disturbances in its immediate vicinity, but there seems to be a slight disturbance in the bottom left.
