This galaxy appears to be an elliptical or lenticular galaxy, displaying a moderately elongated shape. A bright, concentrated central bulge dominates the core region, suggesting an older stellar population is centrally located. Moving outward from the core, the light gradually diminishes with no clear separation in galactic components. The overall color profile indicates a mixture of stellar populations with the central core presenting a yellowish hue, possibly representing older stars. The faint, diffuse halo, which appears slightly bluer than the central region, may host ongoing, yet weak, star formation. The galaxy displays a relatively smooth and continuous light distribution overall, with no prominent spiral arms or distinct features indicative of recent major merger events. Subtle disturbances are potentially visible in the outer halo region on the right side of the galaxy, which may suggest minor gravitational interactions with another object.
