The galaxy presents as a relatively smooth, elliptical-like form with a noticeable elongation along its major axis. The central bulge appears bright and concentrated, exhibiting a yellowish-white hue indicative of an older stellar population. There is a subtle color gradient, with bluer tones observed towards the outer regions of the galaxy, possibly suggesting the presence of younger stars or ongoing star formation in these areas. A smaller, distinct object is located close to the galaxy. It is unclear if the objects are interacting or are simply in the line of sight, but there is a noticeable disturbance to the structure where they are in proximity. Overall, the galaxy's morphology suggests a mature system with a dominant bulge and a relatively quiescent star formation rate.
