The galaxy presents a generally smooth morphology with a slight elongation, appearing cigar-shaped rather than perfectly circular. There are no prominent spiral arms or bar structures visible. The light distribution is centrally concentrated, with the brightest region located at the core. A color gradient is observed, where the central region exhibits a bluer hue, gradually transitioning to a redder color towards the outer edges. There is a hint of some minor disturbance or interaction, but no major merging event is obvious. The overall appearance suggests this is a fairly massive galaxy exhibiting moderate star formation and with a substantial amount of old stellar population.
