The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology. The light distribution suggests a centrally concentrated bulge, with a gradual decrease in luminosity towards the outer regions. The overall shape is slightly elongated, but generally appears rounded. There is no evidence of spiral arms, bars, or significant dust lanes, which supports the classification as an elliptical galaxy. The color of the galaxy is generally yellowish with some bluer regions on the edges, indicating the presence of an older stellar population. The moderate level of star formation rate indicates that some star formation may still be occurring within the galaxy, though at a slower rate than that of spiral galaxies. The galaxy does not seem to be undergoing a major merger or exhibit strong tidal disturbances. There may be evidence of a minor disturbance.
