The galaxy presents an elliptical morphology, appearing relatively smooth and concentrated. Its color profile indicates a predominantly older stellar population, with a yellowish hue dominating the central region, suggesting a lack of significant ongoing star formation. There is little indication of spiral arms or a prominent disk structure. The galaxy exhibits a slight elongation, deviating somewhat from a perfectly spherical shape, with a relatively low probability of being involved in a major merger event based on visual assessment. A very faint blue region is very slightly visible in the outskirts of the galaxy.