The galaxy presents as a relatively smooth, centrally concentrated structure. The light distribution suggests an elliptical morphology, with a high degree of central symmetry. The core region exhibits a bright, yellowish-white hue, indicating a concentration of older stellar populations. Moving outward from the core, the color transitions to a more reddish tone, perhaps reflecting a mix of older stars and dust. There is little evidence of spiral arms or significant dust lanes. There may be a subtle, very faint disk component, but overall the appearance is dominated by a smooth spheroid. There are no immediately obvious signs of any ongoing major merging events, although there is a chance of some minor disturbance as there seems to be very small plume to the top-right of the galaxy. The overall luminosity is substantial, suggesting a massive galaxy.
