The galaxy presents as an elongated, spindle-shaped structure. Its overall appearance is relatively smooth and featureless. There is a noticeable color gradient, with the central region appearing more yellowish-red, possibly indicating a higher concentration of older stars and dust. Towards the outer edges, the color transitions to a bluer hue, which may suggest the presence of younger stellar populations and ongoing star formation activity, albeit at a moderate level. The galaxy exhibits a high degree of ellipticity, appearing significantly longer than it is wide. There is no obvious sign of active galactic nuclei (AGN) activity or major disturbances, such as tidal tails or strong asymmetries. There are also no clear signs of any ongoing major mergers or interactions with other galaxies. The primary axis of elongation is well-defined. Overall, the morphology suggests a relatively evolved system with a dominant spheroidal component.