This galaxy presents as a relatively smooth, elongated structure with an apparent lack of prominent spiral arms or significant dust lanes. The central region exhibits a concentration of light, suggesting a prominent bulge. The overall color gradient shifts from a yellowish-orange core to slightly bluer hues in the outer regions. This suggests a possible gradient in stellar populations, with older, redder stars dominating the central bulge and younger, bluer stars being more prevalent in the galactic disk. There is no obvious evidence of ongoing major mergers, though a slight irregularity in the outer regions might suggest a minor interaction or internal disturbance. The morphology appears to be somewhere between elliptical and lenticular.
