The galaxy appears as a diffuse, elliptical object. The central region exhibits a bright, concentrated luminosity, suggesting a high density of stars in the core. Moving outwards, the light gradually diminishes into a more indistinct halo, indicating a smoother distribution of stellar populations. The overall color profile suggests a population of older stars, emitting light towards the redder end of the spectrum, with a minimal presence of blue, younger stars typically found in actively star-forming regions. The galaxy displays a moderate elongation, indicating a deviation from a perfectly spherical shape. There are no prominent spiral arm structures or significant dust lanes visible in the image. The edges of the galaxy appear smooth and well-defined, without any signs of major tidal disturbances or ongoing merger activity. The galaxy appears to be an isolated elliptical galaxy with minimal signs of recent interactions.
