The galaxy presents as a relatively smooth, elliptical-like structure. It appears centrally concentrated with a bright core, exhibiting a gradient decrease in luminosity towards its outer edges. The light distribution seems largely uniform, lacking prominent spiral arm features or distinct knots of star formation. A slight asymmetry is present; the galaxy is not perfectly circular, hinting at a possible weak tidal interaction or minor disturbance. The color profile suggests a population of older stars, possibly with some intermediate-age stars. There is no obvious dust lane or significant amounts of blue light suggestive of recent star formation. The galaxy's morphological classification most likely leans towards an early-type system.
