The galaxy appears to be an elliptical galaxy, exhibiting a smooth, spheroidal morphology with little to no apparent disk structure. The light distribution is highly concentrated towards the center, suggesting a prominent galactic nucleus. The color gradient transitions from a yellowish-white core to a slightly bluer halo, indicative of older stellar populations dominating the central regions and possibly some younger populations in the outskirts. There is no visible evidence of spiral arms, dust lanes, or ongoing major merging activity. Minor disturbances may be present, but are not readily apparent. The overall structure suggests a well-relaxed system. The estimated size suggests a relatively compact galaxy. The color indices indicate the presence of an evolved stellar population and a low star formation rate.
