The galaxy appears as a centrally concentrated object with a generally smooth morphology. Its color profile indicates an older stellar population, appearing more luminous in redder wavelengths and less so in bluer wavelengths. There is a minimal presence of distinct spiral arms or prominent dust lanes, indicative of a featureless disk. The overall shape approximates an elliptical form, presenting a moderate ellipticity and an overall regular structure with no major disturbances. There is no significant morphological evidence to indicate an ongoing or recent major merger event. The galaxy's high luminosity in all bands suggests a substantial stellar mass, typical of large, evolved systems. The extremely low specific star formation rate implies a galaxy in which star formation is largely quenched, possibly due to morphological or environmental quenching mechanisms. Overall, it appears to be a passive, relatively evolved galaxy with an estimated size of around 5.6 kpc.
