The galaxy presents as a generally smooth, elliptical structure with a marked central bulge. Its shape is moderately elongated, deviating slightly from a perfect sphere. The color distribution shows a concentration of yellow-red hues in the central region, suggesting an older stellar population. Fainter, bluer tints are visible in the outer regions. No prominent spiral arms or dust lanes are discernible within the galaxy's structure, indicating a lack of significant ongoing star formation. The overall appearance suggests a relatively quiescent galaxy with a substantial spheroidal component. There is no evidence of major mergers or significant tidal disturbances.