The galaxy presents a generally smooth, elliptical morphology, appearing largely featureless. There is a slight elongation, though it is mostly rounded in shape. There is no evidence of a distinct disk structure or spiral arms. The light is concentrated towards the center, with a gradual decrease in intensity towards the outer regions. There is no indication of major disturbances such as tidal tails or significant asymmetries, and it does not appear to be undergoing a major merger, although there may be a minor interaction. The galaxy displays a redder hue, suggesting an older stellar population and potentially lower ongoing star formation.
