The galaxy presents as a centrally concentrated object with a relatively smooth overall appearance. Its morphology appears to be that of an elliptical galaxy, displaying a generally rounded shape, with its light profile gradually fading from the bright central region outward. The galaxy exhibits a slight elongation, but no distinct spiral arms or bar structures are discernible. The light distribution suggests a lack of significant dust lanes or patchy star formation regions. There are only minor irregularities, suggesting it is not undergoing any major merging events. The color profile indicates a presence of older stellar populations within the galaxy, with more prominent redder hues dominating the central region. Fainter, bluer colors seem to emanate from the edges of the galaxy.
