The galaxy presents an overall smooth morphology, with a predominantly round shape. The light distribution appears relatively concentrated, with a brighter central region. There is evidence of a potential interaction or merger event, with minor disturbances visible in the galactic structure. The galaxy exhibits a color gradient, transitioning from a bluer hue in the outer regions to a redder hue towards the core. This color variation likely indicates differences in stellar populations, with younger, bluer stars populating the outer regions and older, redder stars concentrated towards the center. The galaxy's size appears moderate. The estimated mass of the galaxy is significant, based on its luminosity and color. The star formation rate is low to moderate, suggesting that star formation activity is present but not dominant.
