The galaxy presents an elliptical morphology with a smooth, diffuse light distribution. The galaxy's central region exhibits a brighter, more concentrated luminosity, suggesting a higher stellar density towards the core. The galaxy's color is primarily a yellow-white hue, hinting at an older stellar population with a relatively low rate of ongoing star formation. The overall shape appears slightly elongated, exhibiting a moderate degree of ellipticity. There's no obvious sign of spiral arms, tidal tails, or significant dust lanes. The galaxy appears largely undisturbed, without any apparent major mergers or interactions. There might be some evidence of minor disturbances in the outer regions, but the overall structure remains primarily smooth and centrally concentrated.