The galaxy presents a generally smooth morphology, though exhibiting some features suggesting potential disturbances. The light distribution appears concentrated towards the center, with a gradual falloff in intensity towards the periphery, indicative of a spherical or elliptical structure. Subtle color variations are observed across the galaxy, with a slightly bluer hue concentrated towards the center, possibly indicating regions of active star formation. However, the outer regions display a redder color, suggesting an older stellar population. Faint asymmetrical extensions or tidal features are observed, hinting at past or ongoing interactions with other galaxies. Overall, the galaxy exhibits characteristics of an intermediate stage system, possibly evolving from a disk-dominated galaxy towards a more elliptical form, potentially due to interactions.
