The galaxy presents as a somewhat elongated, roughly elliptical structure with a concentrated, bright central bulge. It appears relatively smooth, suggesting an older stellar population. There's a subtle hint of asymmetry or minor distortion in the surrounding halo, possibly indicating a past or ongoing minor interaction. The color profile shifts from redder tones in the core to slightly bluer hues in the outer regions. The overall morphology suggests a possible transition stage between elliptical and spiral, perhaps a disk galaxy undergoing transformation.
