The galaxy appears as a slightly elongated, lenticular structure. Its central region exhibits a yellowish hue, indicative of an older stellar population. Moving outwards, a bluer tint becomes more prevalent, suggesting the presence of younger stars within the galactic disc. The galaxy's morphology presents a relatively smooth profile, with no major spiral arms or significant disturbances visible in this observation. A slight distortion is evident, but does not seem to indicate any recent or major merger. The light distribution suggests it is relatively symmetrical and undisturbed.
