The galaxy presents as a relatively smooth and centrally concentrated object. Its overall shape is largely round. The color profile suggests an older stellar population, with a yellowish-red hue dominating the central region, possibly indicating a lack of significant ongoing star formation. Faint blue tinges can be seen in the outer edges suggesting the presence of some younger stars. There is no obvious presence of any strong spiral arm structure or significant dust lanes. The galaxy appears relatively undisturbed, with no obvious signs of a major merger or tidal interactions.
