The galaxy exhibits a generally smooth morphology. The central region is a concentrated, bright yellow, indicating a higher density of older stellar populations. The outer regions have a slightly more diffuse appearance, fading into the background sky. Evident are some disturbances, possibly indicating a recent or ongoing interaction. The galaxy appears to be in a late-stage merger or a close interaction that resulted in significant tidal disruptions. There's possibly a slight elongation or asymmetry in the overall shape, though it's generally elliptical in nature. The colour suggests a relatively low star formation rate compared to blue spiral galaxies, though some ongoing activity cannot be ruled out.
