The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing elongated with a major axis approximately three times the length of its minor axis. The central region displays a yellowish hue, suggestive of an older stellar population. This core region is surrounded by a fainter, bluer envelope, hinting at the presence of some younger stars. The overall structure does not show any prominent spiral arms or significant dust lanes. No obvious signs of a recent major merger event are visible, although some minor irregularities in the outer regions could indicate past gravitational interactions. The galaxy's overall light profile appears relatively even, without sharp discontinuities.
