The galaxy presents a generally smooth morphology, with a slight suggestion of disk-like structure. The central region exhibits a more concentrated luminosity profile, appearing brighter and more compact than the outer regions. There is some irregularity in the shape, hinting at a possible minor disturbance in the gravitational environment. The color distribution suggests a mix of stellar populations, with the central region appearing somewhat redder, potentially indicating a higher concentration of older stars or dust obscuration. The bluer outer regions may indicate more recent star formation activity. There is no strong evidence of a major ongoing merger, though a subtle tidal feature cannot be ruled out. The overall appearance suggests an intermediate stage of galactic evolution, possibly a spiral galaxy undergoing transformation into a lenticular or elliptical type.
