The galaxy appears to be elliptical in morphology, presenting a smooth, largely featureless structure. Its core exhibits a bright, concentrated luminosity, which gradually diminishes towards the outer edges. The color profile suggests a dominant population of older stars, exhibiting a redder hue towards the central bulge and a bluer tint in the peripheral regions. There is no evident presence of well-defined spiral arms or a prominent disk structure. Marginal distortions could indicate minor gravitational interactions.