The galaxy presents a predominantly smooth morphology, indicative of an elliptical or lenticular type. Its light distribution is centrally concentrated, with a gradual decrease in intensity towards the outer regions. The core appears bright and somewhat diffuse, with no readily discernible substructure. The object exhibits a generally round shape, though some slight deviations from perfect circularity are present. No evidence of spiral arms, dust lanes, or significant tidal disturbances is apparent. The galaxy exhibits a redder color, suggesting an older stellar population and minimal ongoing star formation. The estimated size of the galaxy is moderate, as it subtends a small, but not insignificant, angular extent in the image. Overall, the galaxy's characteristics suggest a relatively quiescent system with minimal recent interaction or star-forming activity.
