The galaxy presents a generally smooth, elliptical morphology. The core region appears to be a bright, relatively homogenous distribution of light, suggesting a concentrated stellar population. The overall color profile is indicative of a relatively old stellar population, with a slightly reddish hue dominating. There is a subtle transition from the brighter core to a fainter, more diffuse halo region. No prominent spiral arms or distinct dust lanes are visible. The galaxy exhibits a degree of roundness that leans towards elliptical, with a small deviation from a perfectly circular shape. There are no indications of major mergers or significant tidal disturbances in its immediate vicinity. The surrounding halo exhibits some faint, diffuse light, without any clear signs of recent star formation. Overall, the galaxy appears to be an evolved system, likely dominated by older stars.
