The galaxy presents as a generally smooth, elliptical-like object with a concentrated central bulge. The core region exhibits a distinct yellowish-red hue, suggesting an older stellar population dominated by red giant stars and potentially a significant dust presence. Fainter bluish extensions are observed towards the outer regions of the galaxy. While these extensions are not highly defined, they suggest the presence of younger, hotter stars, possibly indicative of ongoing, low-level star formation activity. No prominent spiral arm structures or significant dust lanes are visible. The overall morphology appears relatively undisturbed, although a hint of asymmetry could be present on the left side.
