The galaxy presents a predominantly smooth morphology. There is a slight asymmetry, possibly indicative of a minor interaction or internal disturbance. The central region exhibits a concentrated luminosity, suggesting a prominent galactic nucleus. The color profile transitions from a yellowish-white core to a slightly redder halo, potentially indicating an older stellar population in the outer regions. No distinct spiral arms or bar structures are clearly discernible. Overall, the galaxy appears to be relatively evolved and quiescent, with minimal evidence of active star formation based on color. The estimated size suggests it is a relatively compact galaxy.
