The galaxy presents as a well-defined, elongated structure. The morphology appears largely smooth, with a central bulge that exhibits a yellowish-orange hue. Moving outward from the center, the color shifts towards a bluer tone in the outer regions. The pronounced cigar shape indicates a possible classification as an elliptical galaxy, viewed edge-on. There is no indication of a strong central bar structure or prominent spiral arms. The slight blue tinge in the outer edges suggests the presence of some ongoing star formation, although this activity seems subdued compared to that observed in actively star-forming spiral galaxies. There are no indications of a major merger event or significant tidal disruption, although subtle asymmetries or minor disturbances cannot be entirely ruled out based on this image alone. Overall, the galaxy appears to be a relatively quiescent system, likely dominated by older stellar populations in the central region.
