The galaxy presents as a centrally concentrated, luminous object with a generally smooth appearance. Its color profile indicates a population of older stars, with a redder hue concentrated in the central bulge and a slightly bluer component extending towards the outer regions of the galaxy. The morphology suggests that it is likely an elliptical galaxy, or possibly a lenticular galaxy seen at a slight angle. No distinct spiral arm structures or prominent dust lanes are visible. The galaxy exhibits a relatively high degree of rotational symmetry, appearing mostly undisturbed, with only minor indications of any past or ongoing merger activity. The light distribution is fairly even, diminishing gradually from the core outwards.
