The galaxy exhibits a generally smooth morphology, with a relatively high degree of central concentration. The overall shape appears somewhat rounded, lacking any pronounced elongated or irregular features. There is very little evidence of a disk component or spiral arms. The color profile suggests a population of older stars, with a slight reddening effect due to its distance. No significant signs of ongoing mergers or tidal disturbances are apparent. Based on the morphology and color, this galaxy is likely an elliptical galaxy, possibly residing somewhere between an intermediate mass and a massive system. The low rate of current star formation activity reinforces this assessment. 
