The galaxy appears to be a relatively smooth, elliptical-like structure. The galaxy exhibits a yellow-orange hue, which suggests an older stellar population and reduced on-going star formation. The central region of the galaxy is noticeably brighter and more concentrated. The overall shape seems to be somewhere between round and elongated. There is a suggestion of a possible tidal interaction or merger event, potentially with faint structures extending outwards, although the image quality makes it difficult to confirm definitively. These structures may be minor disturbances. Overall, the galaxy presents a morphology consistent with a moderately massive system, likely in a relatively quiescent state.
