The galaxy presents as an elongated, cigar-shaped system. It appears to be an early-type galaxy, likely an elliptical or lenticular, characterized by a smooth, centrally concentrated light profile. The core region exhibits a yellow-orange hue, suggesting an older stellar population dominating the inner regions. Moving outward from the core, a subtle bluish tinge is visible, possibly indicating a younger, albeit small, population of stars or residual star formation activity in the outer disk or halo. No distinct spiral arm structures or prominent dust lanes are discernible. The overall morphology suggests a relatively evolved galaxy with a significant fraction of its stellar mass already formed. There are no obvious signs of ongoing major mergers or strong tidal interactions; the structure appears relatively undisturbed, though subtle disturbances may be present.
