The galaxy presents as a fairly smooth, elliptical-like structure with a centrally concentrated brightness profile. There appears to be a slight elongation, deviating from a perfectly circular shape; the galaxy appears to be somewhat in between round and cigar shaped. The color profile suggests an older stellar population, showing a dominant yellowish-white hue in the central region which could be due to older, redder stars. The outer regions display a subtle bluer tinge, potentially indicating the presence of younger stars but this is relatively faint. There is also a very small object that could be part of the galaxy or an interaction. There's no clear indication of spiral arms, bar structures, or significant dust lanes. The overall morphology suggests a mature galaxy with little evidence of recent major mergers or disturbances. Star formation activity is likely low.
