The galaxy presents as a moderately luminous, elongated structure. The central region exhibits a high surface brightness with a yellowish-white hue, suggestive of an older stellar population. Moving outward from the core, the galaxy displays a diffuse, bluish halo, hinting at the presence of younger, hotter stars and possible ongoing star formation. The overall morphology appears relatively smooth, though there is a slight irregularity in the outer regions, potentially indicating minor disturbances. The lack of clearly defined spiral arms suggests a disk galaxy with a dominant bulge, possibly an S0 or early-type spiral. There is no strong evidence of an ongoing major merger event.
