The galaxy presents as a relatively smooth, elliptical-like structure. There is a bright, concentrated central region with a general yellow-orange hue, indicative of an older stellar population. The light distribution fades gradually outwards from the center, lacking any distinct spiral arms or prominent star-forming regions. The shape appears elongated, suggesting a degree of ellipticity rather than a perfectly circular form. Minimal dust lanes or other obscuring features are apparent. There are no obvious signs of major mergers or tidal disturbances. The galaxy appears to be relatively isolated.
