The galaxy presents as a fairly compact, elliptical structure with a smooth, concentrated light profile. The dominant color appears to be yellow-orange, suggesting an older stellar population with relatively low ongoing star formation. The overall shape is nearly circular, exhibiting minimal evidence of disk-like features or significant tidal disturbances. There is no clear indication of a recent or ongoing major merger event. Subtle color variations across the galaxy suggest the presence of slight differences in the age or metallicity of the stellar population. The apparent size of the galaxy is relatively small, indicating a considerable distance.
