This galaxy presents a primarily smooth morphology, appearing largely featureless with an elliptical shape. Its color profile indicates a higher concentration of older stellar populations, leaning towards redder wavelengths. While generally appearing as a single, cohesive structure, there is a suggestion of some minor disturbance in the morphology, potentially indicating a past or ongoing interaction. The galaxy exhibits a moderate degree of roundness, lacking a pronounced disc structure. Evidence suggests that the galaxy may be in the process of merging or have recently undergone a minor merger event.