The galaxy presents as a relatively compact, lenticular-like system. There appears to be a central, luminous bulge dominating the overall structure, with a smoothly decreasing brightness profile outwards. Subtle, disk-like features are suggested, though not distinctly resolved. The galaxy exhibits a color gradient, transitioning from a bluer core region, possibly indicating recent or ongoing star formation, to slightly redder, more quiescent outer regions. Faint hints of spiral structure may be present in the form of subtle color variations and asymmetries within the disk component. There's no clear evidence of strong tidal interactions or major disturbances, suggesting it is a relatively isolated system undergoing steady-state evolution, although there may be some minor disturbance.
