The galaxy presents as a single, relatively smooth object, although its morphology is not entirely uniform. There is a brighter, more concentrated central region that appears yellowish-white, possibly indicating an older stellar population and less active star formation within the core. A fainter, round area is separate from the core, and it suggests a possible ongoing merger event or tidal interaction with another smaller galaxy. The overall shape can be described as moderately round, with a hint of asymmetry, possibly due to the gravitational interactions. There is a distinct lack of spiral arm structures or prominent dust lanes, suggesting it may be an elliptical galaxy or a disk galaxy viewed at an angle where spiral structures are not easily discernible. The galaxy exhibits a reddish hue overall, indicating a population of older stars.
