The galaxy presents as a relatively smooth, elongated structure, suggestive of an elliptical morphology. The light distribution appears concentrated towards the center, with a gradual decrease in intensity moving outwards along the major axis. The color profile is predominantly yellow-orange, indicating an older stellar population with limited ongoing star formation. The pronounced elongation, exhibiting a cigar-like shape, suggests it is an elliptical galaxy. There is no readily apparent evidence of spiral arms or distinct features such as dust lanes. No signs of a recent major merger are visible. Small irregularities are consistent with minor gravitational interactions or disturbances. Overall the morphology suggests a lack of significant recent interactions.
