The galaxy presents a roughly elliptical morphology. Its central region displays a bright, smooth appearance, indicative of a significant stellar population density. Moving outwards, the galaxy exhibits a diffuse halo characterized by a mixture of colors. Predominantly, a yellowish-red hue is observed within the halo suggesting the presence of older stellar populations. There are indications of some faint, blue regions, perhaps indicative of younger stellar formation activity, though they appear localized and minimal. There is visible distortion in the general shape of the galaxy with some irregular features. The overall visual impression is that of a system undergoing some form of interaction or internal disturbance which is likely minor. The luminosity profile appears to decline smoothly from the core, with no sharp edges or pronounced spiral arms.