The galaxy appears to be a relatively smooth, elliptical galaxy at a redshift of approximately 0.138. The light distribution is centrally concentrated, exhibiting a high degree of radial symmetry and lacking any obvious spiral arm structure or distinct features such as dust lanes. The galaxy's shape is generally round, with only a very slight elongation. It displays a color gradient, transitioning from a bluish-white core to a more yellowish-red halo, suggesting a population of older stars in the outer regions and potentially ongoing, low-level star formation within the central region. There is no evidence of any major ongoing merger events or significant tidal disturbances affecting the galaxy’s morphology. Based on the light profile and overall appearance, this galaxy is likely an early-type galaxy with a high degree of sphericity and a stellar mass of approximately 10^9.8 solar masses. Star formation rate appears to be relatively low.
