The galaxy presents as a somewhat smooth, elliptical structure with a high degree of central concentration. The core exhibits a yellowish hue, suggesting an older stellar population and reduced ongoing star formation in that region. There is a hint of a faint, extended disk or halo surrounding the central bulge, contributing to the overall size. This disk exhibits a bluer tint, potentially indicative of younger, hotter stars and active star formation within these outer regions. There is a slight asymmetry in the distribution of light, which may suggest a past or ongoing minor interaction or merger event. Overall, the galaxy appears relatively undisturbed, with no prominent tidal tails or other signs of major disruption.
