The galaxy exhibits a distinct but somewhat irregular morphology. It appears centrally concentrated, with a bright core. Evidence of a disk-like structure is present, though somewhat disturbed. The galaxy displays a range of colors, transitioning from a bluer hue in the central regions, possibly indicative of ongoing star formation, to redder tones in the periphery. Some asymmetry is apparent in the distribution of light, with a more defined extension towards one side. This could be indicative of tidal interactions or a recent merger event. The galaxy's light profile is generally smooth, suggesting an older stellar population, but some faint, patchy features might be present. Overall, the galaxy presents characteristics of a system that has experienced some form of disturbance or interaction, yet retains a degree of structural coherence.
