The galaxy presents as a somewhat elliptical, smooth object with a concentrated central bulge exhibiting a yellowish hue. This suggests an older stellar population dominating the core. The outer regions fade into a less defined halo, showing a subtle gradient of redder tones, potentially indicative of ongoing, albeit diminished, star formation activity in the outer reaches or a population of older, redder stars. There is a slight asymmetry to the object, suggesting a possible recent interaction, or perhaps just an uneven distribution of stellar material. Overall, the galaxy appears to be relatively evolved, consistent with a transitioning, possibly quenching, spiral or an elliptical galaxy.
