The galaxy presents as a relatively smooth, elliptical-like structure. It is generally round in appearance, with no obvious spiral arms or a distinct disk component visible in the image. A possible concentration of light may be present towards the center, suggesting a higher density of stars in the galactic nucleus. The galaxy exhibits a yellow-red hue, indicative of an older stellar population with diminished ongoing star formation. There appears to be a possible minor disturbance in the structure, suggesting a prior interaction. The galaxy appears to be in a relatively isolated region of space.
