The galaxy presents a somewhat elliptical morphology, exhibiting a concentrated central bulge with a diffuse halo extending outwards. The core appears luminous with a yellowish-white hue, indicative of an older stellar population. The surrounding region displays a bluer tint, suggesting the presence of younger stars, although the overall star formation rate seems relatively low. There's a subtle disk-like structure implied in the broader distribution of light, but it lacks well-defined spiral arms. The galaxy doesn't show any major signs of interaction or merging, although there may be some minor disturbances or asymmetries in the outer regions. The galaxy seems relatively isolated and undisturbed in its evolution.
