The galaxy exhibits a concentrated central bulge with a moderate degree of ellipticity. It appears relatively compact, with an estimated effective radius of approximately 4 arcseconds. There are indications of a possible disk-like structure surrounding the bulge, as suggested by the overall shape. The color profile transitions from a brighter, bluer core to redder outer regions, potentially indicating a difference in stellar populations or dust extinction. There appears to be evidence of minor disturbances in the galaxy's morphology, which might indicate a prior or ongoing minor merger event. The galaxy shows a complex color gradient, with a significantly brighter intensity in the center. The overall light distribution suggests an object that is relatively smooth, but some faint features are noticeable that point towards some kind of interaction.
