The galaxy presents a primarily smooth, elliptical morphology. The central region exhibits a concentrated, bright core, indicative of a substantial stellar population. Moving outwards from the core, the light intensity diminishes gradually, transitioning to a fainter, diffuse halo. A subtle asymmetry is observed in the outer regions, possibly hinting at minor tidal interactions or past accretion events that have not significantly disrupted the overall smooth structure. No distinct spiral arms or prominent dust lanes are discernible in this image. The color appears predominantly yellowish, suggesting an older stellar population with lower rates of ongoing star formation. The galaxy is generally well-defined, with a soft, indistinct edge where it fades into the background.
