The galaxy presents a somewhat elliptical morphology with a smooth, diffuse appearance. It exhibits a central bulge that appears relatively bright and concentrated, gradually fading into a less defined disk. The color profile suggests a relatively mature stellar population, indicated by a redder hue in the disk, contrasting with a slightly bluer central region, potentially pointing to ongoing, or more recent star formation in the core. There is some indication of minor disturbances or tidal features potentially suggesting past or ongoing interactions with other galaxies. There seems to be an asymmetric distribution of light and some subtle indications of faint features surrounding the main body of the galaxy. The galaxy does not appear to exhibit strong spiral arm structures.
