The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light distribution. There is a subtle elongation, hinting at a possible deviation from perfect sphericity. The color profile appears relatively uniform, with a slight concentration of yellow and white light toward the core, likely indicating an older stellar population. There's no indication of prominent spiral arms, dust lanes, or intense star-forming regions in the visible spectrum. The overall structure seems undisturbed, with no obvious signs of recent major mergers or tidal interactions. The galaxy appears to be relatively isolated in its environment.
