The galaxy presents as an elongated, somewhat irregular structure. A central, brighter region exhibits a reddish-orange hue, potentially indicative of an older stellar population with lower rates of star formation and dust obscuration. Extending outwards from this central region are fainter, more diffuse structures. Hints of bluer colors are visible in these outer regions, suggestive of younger, hotter stars and ongoing star formation, though at a low overall rate. The galaxy appears to be undergoing some form of interaction or disturbance, as evidenced by its asymmetry and possible tidal features. The overall morphology suggests a system that is neither purely elliptical nor a well-defined spiral, but instead a transitional or disturbed form, possibly a late-stage spiral galaxy undergoing transformation. There appears to be a moderate degree of internal smoothness, with only subtle indications of more complex substructure such as spiral arms. Some distortion may have been caused by a past merger event.
