The galaxy exhibits a primarily elliptical morphology with a high degree of central concentration. It presents a smooth, symmetrical light distribution, suggesting a lack of significant spiral arm structures or prominent dust lanes. The color profile indicates a yellowish-red hue, which could be attributed to an older stellar population or the presence of dust obscuration. The galaxy appears relatively isolated, with no obvious signs of ongoing major mergers or tidal interactions. There is a slight hint of a less concentrated region to the lower right, it is unclear if this is part of the galaxy or a separate object. The overall structure is consistent with a galaxy that is in a relatively quiescent state of evolution.
