The galaxy presents as a somewhat compact, luminous entity with a smooth and largely featureless morphology. Its overall shape appears round or slightly elliptical. The central region exhibits a higher concentration of luminosity, suggesting a prominent galactic nucleus. There is a color gradient observable, shifting from a yellowish-white core to a redder hue in the outer regions, potentially indicating a difference in stellar populations, with older stars located at the periphery. There are no apparent spiral arm structures or dust lanes visible within the galaxy. There is no evidence of any ongoing major merging activity or tidal disturbances. The estimated size of the galaxy is several kiloparsecs across. Overall, the galaxy has the appearance of a typical elliptical or lenticular galaxy. The star formation activity appears to be very low.