This galaxy presents as a relatively smooth, elliptical morphology. The light is concentrated towards the center, exhibiting a bright, yellowish core. Moving outward, the luminosity gradually decreases, transitioning into a fainter, diffuse halo. The overall shape is elongated, appearing more lenticular than perfectly spherical. There is a subtle suggestion of a disk-like structure, although no distinct spiral arms or prominent dust lanes are discernible within the available image resolution. I see no obvious signs of ongoing major merging activity, however, a small disturbance may be present. The overall impression is of a mature galaxy, likely with a relatively low star formation rate.
