The galaxy presents as a somewhat elongated, disk-like structure. Its core exhibits a concentrated, bright yellow-white luminosity, suggesting a dense population of older stars. Moving outward from the central region, the light intensity gradually decreases into a less luminous, more diffuse halo. The morphology indicates a relatively smooth structure with a subtle disk, lacking prominent spiral arms or distinct features such as dust lanes. The shape shows some signs of elongation, potentially indicating a mild disturbance or tidal interaction in its past, though it primarily resembles a somewhat rounded disk. Overall, the galaxy appears to be a relatively quiescent system.
