The galaxy presents as a moderately bright, elongated, disk-like structure, with an aspect ratio suggesting a significant inclination relative to our line of sight. The central region exhibits a strong concentration of light, appearing smooth and featureless, consistent with a substantial bulge component. The color profile indicates a redder central bulge which could point to a population of older stars. The outer disk appears bluer and contains younger stars. No prominent spiral arm structure or dust lanes are readily discernible in this image, possibly due to the image resolution or the galaxy's morphological type. There is no apparent interaction or tidal disturbance. The overall morphology suggests a relatively quiescent galaxy, with no signs of major ongoing mergers.
