The observed galaxy appears as a relatively smooth object. It exhibits a concentrated central region that fades into the surrounding space. The morphology is largely elliptical in shape, with no apparent spiral arm structures or significant dust lanes visible. The color profile suggests the presence of an older stellar population, with a subtle reddish hue indicating a lack of recent star formation. There is a slight asymmetry in the outer regions of the galaxy, possibly indicating a minor gravitational interaction or past merger event. However, the primary structure remains largely undisturbed, without any major tidal tails or significant distortions. 
