The galaxy presents as a relatively smooth object with a somewhat elliptical shape. A central bulge is visible, exhibiting a brighter, more concentrated luminosity than the surrounding regions. The light distribution gradually decreases with radial distance from the center, fading into the background sky. The galaxy appears to have a slight tilt relative to our line of sight. There is a subtle elongation in the overall form, with a hint of a disk-like structure present, though it appears mostly smooth. No distinct spiral arms or prominent dust lanes are apparent in this image. The color profile suggests an older stellar population with a general lack of blue color, and some areas are redder, perhaps indicating older stars. There may be minor distortions in the galaxy's overall shape.
