The galaxy presents as a centrally concentrated object with a roughly elliptical morphology. The core exhibits a bright, yellowish hue, suggesting an older stellar population and potentially lower star formation activity. A faint, plume-like extension emanates from the central region, displaying a more greenish tint, possibly indicating regions of ongoing or recent star formation. This feature appears somewhat disturbed, hinting at a possible interaction or recent merger event. Overall, the galaxy appears to be relatively smooth and not highly structured, with a moderate degree of roundness. There is no obvious spiral arm structure visible. The integrated color suggests a significant population of evolved stars, consistent with a substantial stellar mass.
