The galaxy appears as a relatively smooth, elliptical structure. There is a noticeable concentration of light towards the galactic center, indicative of a bulge. The color profile suggests a population of older stars, with a redder hue dominating. No distinct spiral arms or significant dust lanes are visible. The overall morphology suggests a quiescent galaxy, possibly with low ongoing star formation. There is no obvious evidence of recent major merger activity or significant tidal disturbances. The galaxy exhibits a generally round shape. 
