The galaxy presents as a yellowish, elliptical form with a smooth light distribution, exhibiting a relatively high degree of central concentration. The overall shape appears mostly round but slightly elongated. No distinct spiral arms or bar structures are discernible. There is no indication of significant tidal disruption or ongoing major merger events. Subtle hints of internal structures suggest the possibility of a central bulge with an extended, fainter halo. The color suggests a population of older stars with only low levels of ongoing star formation activity. There are no prominent dust lanes or bright star-forming regions visible.
