The galaxy presents a relatively smooth and featureless morphology. Its shape appears elongated, approximately cigar-shaped, with a gradual increase in surface brightness toward the central region. The color profile indicates a slightly redder hue overall, suggesting a population of older stars. There may be minimal star formation activity occurring within the galaxy. No obvious signs of spiral arms, bars, or dust lanes are apparent in the image. The galaxy exhibits no strong signs of interaction or tidal disturbances.
