The galaxy presents as a moderately bright, elliptical or lenticular type. It appears to be primarily smooth in texture with a concentrated central bulge that exhibits a yellowish hue, suggesting a population of older stars. Surrounding the bulge, the galaxy displays a fainter, more diffuse disk. The disk shows a bluer tint than the central bulge, possibly indicating the presence of younger stars. The overall shape is slightly elongated, showing moderate ellipticity with no obvious spiral arm structure or dust lanes visible in this resolution. There are hints of some minor disturbances or asymmetries in the outer regions of the disk. The galaxy appears relatively isolated, showing no immediate signs of a major merger event.