The galaxy presents an overall disk-like morphology, though with a relatively indistinct spiral structure. The disk appears inclined to our line of sight. There's a central bulge that appears relatively prominent. The color profile indicates a relatively blue hue overall, suggesting ongoing star formation. No signs of a major merger are apparent, and the disk doesn't appear significantly disrupted, though minor disturbances can't be ruled out. The galaxy's light is concentrated towards the center, gradually fading into its outer regions. The overall size of the galaxy is intermediate.
