The galaxy presents a largely smooth, elliptical morphology. Its light profile is highly concentrated towards the center, with a gradual decrease in brightness moving outwards. The core region exhibits a yellowish-white hue, indicative of an older stellar population. There is very little evidence of spiral arm structures or significant dust lanes. The overall shape is nearly round with only slight elongation. The galaxy appears relatively undisturbed, showing no obvious signs of ongoing major merging activity. Faint blue-ish emission is present on the outer edges, perhaps indicating some sparse recent star formation. The mass is concentrated at the center. Overall, the galaxy presents an elliptical morphology with hints of recent star formation activity.
