The galaxy presents as a spiral galaxy, inclined somewhat to our line of sight. The central bulge appears prominent and moderately bright, with a yellowish hue. The disk component shows a somewhat flocculent structure, possibly exhibiting spiral arm segments. There may be presence of a faint bar-like feature across the bulge, extending into the inner disk region. The overall color of the disk is bluer than the bulge, suggestive of ongoing star formation within the spiral arms. No major signs of tidal disruption or interaction with other galaxies are immediately apparent. The galaxy shows a clear central concentration of light, indicative of a well-formed bulge component within a rotating disk.
