The galaxy presents as a spiral, viewed at a moderate inclination. The nucleus appears bright and somewhat diffuse. A distinct disk is visible, though not perfectly symmetrical, potentially indicating a minor gravitational interaction. The disk shows some evidence of structure, possibly faint spiral arms, though these are not sharply defined. There may be some signs of dust lanes along the disk. One region on the disk appears brighter than others, possibly indicating an area of star formation. A notable feature is a somewhat detached luminous region situated toward one end of the major axis, suggestive of a tidal tail or a smaller merging companion. The overall color suggests a mix of stellar populations, with the nucleus and disk having a relatively redder hue, while the brighter region on the disk has a slightly bluer color, possibly indicative of ongoing star formation. The estimated size of the galaxy is moderately large.
