The galaxy presents a generally smooth, elliptical morphology. There is a notable concentration of luminosity towards the galactic center, displaying a bright, yellowish core. Moving outwards from the core, the light gradually diffuses into a fainter, more reddish halo. The overall shape appears to be moderately elliptical, showing a slight elongation rather than perfect circularity. No distinct spiral arms or prominent dust lanes are discernible within the observed structure. The lack of significant irregularities suggests that the galaxy is not currently undergoing a major merger event, though minor disturbances cannot be ruled out based on visual inspection alone. The color profile suggests a population of older stars, with relatively little evidence of ongoing active star formation.
