The galaxy presents a generally smooth morphology, with a high degree of central concentration. The light profile suggests a centrally dominant spheroid. The galaxy appears predominantly elliptical in shape, with a high degree of roundness. There is no apparent spiral arm structure, and no strong evidence of recent merger activity. The color index suggests a relatively evolved stellar population, likely dominated by older, redder stars, with a moderate amount of dust extinction. Star formation appears to be relatively quiescent, with only a low level of activity. The absolute magnitude indicates a luminous galaxy.
