The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge that gradually fades into the outer regions. The color profile is dominated by yellow hues in the core, suggesting an older stellar population. The galaxy's overall shape is neither perfectly spherical nor highly elongated, with a moderate degree of ellipticity. There is no obvious sign of strong spiral arm structure. The galaxy is relatively undisturbed, with no prominent tidal features or indications of a major ongoing merger. There might be hints of minor disturbances, but these are not strongly pronounced. The size of the galaxy appears moderately large. Based on the data, we can assume the galaxy is experiencing some degree of star formation, albeit potentially at a relatively low rate.
