The galaxy appears to be an elongated, likely spiral or lenticular, system with a smooth overall texture. The central region exhibits a bright, concentrated luminosity, suggesting a substantial bulge component, or possibly an active galactic nucleus. The color gradient transitions from a yellowish core to slightly bluer hues in the outer regions, possibly indicating more recent star formation in the disk. The galaxy does not display strong evidence of spiral arm structure, it seems to be a relatively evolved system. It doesn't appear to be heavily disturbed or undergoing a major merger. There are no obvious tidal tails, indicating a lack of recent major interactions.
