The galaxy presents a generally smooth, elliptical morphology. The light profile appears centrally concentrated, with a gradual decline in intensity towards the outer edges. The galaxy exhibits an overall yellowish-white hue, suggesting a stellar population dominated by older, redder stars. A subtle elongation is observable, deviating from a perfectly circular shape. There may be a hint of a faint disk-like structure, but further observations are needed to confirm this. No obvious signs of spiral arms or active star formation regions are visible in this image, but there could be a small amount of star formation. There are no signs of any major mergers in the morphology of this galaxy.
