The galaxy presents as an elliptical morphology, elongated in shape. The central region is a bright, concentrated core exhibiting a yellowish-orange hue, suggesting an older stellar population and possibly a high density of stars. Moving outward from the core, the intensity of light gradually diminishes. A faint bluish tinge around the edges implies the presence of a small population of younger, hotter stars, although their contribution to the overall light appears minimal. There is no discernible spiral structure or prominent dust lanes. The galaxy appears relatively undisturbed with no clear signs of ongoing major mergers or tidal interactions. 
