The galaxy presents as a relatively smooth, elliptical structure with an apparent disk. Its shape is elongated, displaying a cigar-like appearance rather than a perfectly circular form. The galaxy's core exhibits a bright, concentrated region of light, suggesting a dense stellar population or active galactic nucleus. Moving outward from the core, the luminosity gradually diminishes, indicating a decreasing stellar density. While the galaxy appears mostly smooth, there are subtle hints of minor disturbances or irregularities in its outer regions, potentially indicating past interactions with other galaxies or internal dynamic processes. The overall color profile suggests a mix of stellar populations, with the inner regions potentially dominated by older, redder stars, while the outer regions may contain younger, bluer stars. No distinct spiral arm structures or dust lanes are readily apparent. The galaxy appears to be in a relatively evolved state, with ongoing, albeit moderate, star formation.
