The galaxy presents as a concentrated, elliptical-shaped structure with a smooth overall appearance. Its central region exhibits a bright, yellowish hue, indicative of an older stellar population likely dominated by evolved stars. Moving outwards from the core, the galaxy gradually fades into a less defined outer halo, showing a slight bluish tint which may signify the presence of younger, hotter stars, or potentially ongoing, albeit low-level, star formation. No distinct spiral arms or other prominent features are discernible. The galaxy appears relatively undisturbed, with no strong evidence of recent mergers or tidal interactions.
