The galaxy presents as a centrally concentrated object, appearing smooth in texture with a largely elliptical morphology. The central region exhibits a strong concentration of luminosity, with a radial decrease in surface brightness towards the outer edges. The color profile is dominated by yellow and orange hues, indicating a stellar population that is primarily older and less actively forming stars. There is some evidence of blue light in the surrounding areas, indicating the possibility of ongoing, but likely low levels of star formation, within its extended regions. No distinct spiral arms or bars are discernible, and the galaxy does not appear to be undergoing any major mergers, though there is a subtle irregularity in the galaxy's shape, hinting at a possible recent minor interaction.
