The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. There is a noticeable color gradient, transitioning from a yellowish-white core to a reddish outer halo. The galaxy shows little evidence of spiral arm structure or prominent dust lanes, suggesting it may be an early-type galaxy. The smooth light distribution and lack of significant morphological disturbances indicate that it is likely a relaxed system, without recent major mergers. There is a slight elongation in its shape, deviating from a perfectly circular form. The overall appearance implies a galaxy dominated by an older stellar population, with relatively low ongoing star formation.
