The galaxy presents as a well-defined elliptical structure with a dominant central bulge. The light profile is smooth, exhibiting a relatively uniform distribution of luminosity across its extent, with a slight increase towards the core. The object appears elongated, exhibiting an asymmetry. There is no significant evidence of spiral arm structures or distinct dust lanes within the observed wavelengths. A faint halo of diffuse light is present extending beyond the main body of the galaxy, suggesting a population of older stars. Based on its general morphology, the galaxy seems to be an evolved system with a relatively low current star formation rate. There appears to be no major mergers occurring.
