The galaxy presents as a luminous, somewhat elliptical object. The light profile suggests a smooth distribution of stars, with a concentration of luminosity towards the center, exhibiting a central bulge. The overall color appears to be more weighted towards the redder end of the spectrum, possibly indicating an older stellar population. There might be some ongoing, albeit limited, star formation. The galaxy does not appear to be highly disturbed, although some minor irregularities in shape cannot be ruled out based on the resolution. It appears as though it is relatively isolated, without any strong indications of recent major merger events. It is primarily a smooth, round object with a red hue.
