The galaxy appears as a fairly smooth, centrally concentrated object with a slightly elliptical morphology. The color profile suggests an older stellar population, exhibiting a yellowish-orange hue in the central regions. There is little evidence of spiral arm structure or significant dust lanes within the observable light. The overall appearance indicates a relatively quiescent galaxy, possibly an early-type spiral or an elliptical galaxy transitioning into a more passive state. There may be signs of a slight tidal disturbance or minor interaction in the shape of the galaxy, however, the dominant appearance is of a stable system.