The galaxy appears as a concentrated, elliptical-like structure, exhibiting a relatively smooth morphology. There is a significant central bulge that dominates the light output. The galaxy presents a yellowish-red hue, indicating an older stellar population and/or significant dust obscuration. There is no apparent spiral arm structure or evidence of active star formation regions visible in this image. The galaxy has a somewhat regular shape, though a slight asymmetry is visible. It does not display any prominent tidal features or signs of a major ongoing merger event. Based on the colors, it is plausibly a relatively massive galaxy.
