The galaxy presents as a lenticular system, viewed at an oblique angle to its equatorial plane, exhibiting a moderate ellipticity. It shows a central bulge region appearing yellowish-white, indicative of an older stellar population. A faint, bluish disk surrounds the bulge, suggesting the presence of some younger, hotter stars and ongoing star formation. Dust lanes or patchy structures are not readily discernible in this image, leading to a relatively smooth appearance. The overall color gradient from the center to the outer regions suggests a radial population gradient, with older stars concentrated towards the core and bluer, younger stars more prevalent in the disk. 
