The galaxy presents a generally smooth, elliptical morphology. Its core exhibits a concentrated luminosity, transitioning outwards into a more diffuse halo. The colour profile suggests a population dominated by older stars, exhibiting a reddish-yellow hue that becomes more pronounced towards the core. There's a subtle flattening of the galaxy's shape, hinting at a possible oblate spheroidal structure, but no distinct spiral arm features or dust lanes are apparent. No signs of ongoing major merger activity are observed, although there is a very slight asymmetry which could suggest a minor gravitational disturbance. Overall, the galaxy appears to be a relatively evolved system with a significant stellar mass.
