The galaxy presents as a moderately bright, elliptical-like structure, exhibiting a smooth, diffuse morphology. The core region demonstrates a concentrated luminosity, decreasing in intensity outwards with a subtle gradient. The galaxy appears somewhat elongated with the major axis oriented approximately northwest to southeast. There's a lack of distinct spiral arm features or prominent dust lanes visible within the observed wavelength range. The overall color suggests a relatively evolved stellar population, potentially indicative of reduced ongoing star formation. There is a possibility of some minor disturbances due to the slight asymmetry that is observed, however it is likely a normal elliptical galaxy.
