The galaxy appears as a relatively smooth, elliptical-like structure. Its central region exhibits a concentrated, bright luminosity, suggesting a significant stellar density or potentially an active galactic nucleus. The overall color profile leans towards the redder end of the spectrum, indicating an older stellar population and lower rates of on-going star formation activity. The galaxy presents a slightly elongated shape, with its isophotes appearing mostly regular, suggesting the galaxy is in a relatively relaxed state. There is no apparent spiral arm structure or significant dust lane obscuration visible. The galaxy exhibits a high degree of central concentration, with the majority of its light emitted from the core region. There are minimal signs of tidal disturbances or interactions with neighboring galaxies.
