The galaxy presents as a generally smooth and rounded structure. The light profile exhibits a strong central concentration, indicative of a prominent galactic bulge or core. The color gradient suggests a radial variation in stellar populations, with the core appearing yellower, possibly due to older stars, and the outer regions showing hints of bluer colors, potentially indicative of younger stellar populations and ongoing star formation, although this activity appears to be at a low level. There is no apparent spiral arm structure or significant dust lane obscuration visible. Faint disturbances or minor features may be present, but there is no evidence of a major merger event in the recent past. The overall morphology suggests the galaxy may be an early-type spiral or lenticular galaxy, potentially on its way to becoming a elliptical galaxy.
