The galaxy presents as a relatively compact, centrally concentrated object. It exhibits a dominant spheroidal morphology with a smooth light distribution, lacking prominent spiral arm structures. The color profile indicates a population of relatively older stars. There is no clear evidence of a significant dust lane or ongoing major star formation within the visible region. The overall structure appears undisturbed, with no apparent signs of recent major merger events. The galaxy's apparent roundness suggests it is viewed relatively face-on. However, there is faint evidence of minor disturbances, possibly hinting at past interactions or minor mergers.
