The galaxy presents as an elongated, cigar-shaped structure with a relatively smooth appearance. The color gradient suggests a redder core region, transitioning to slightly bluer hues along the outer edges, hinting at ongoing or recent star formation in these areas. No distinct spiral arms or prominent dust lanes are discernible, suggesting a galaxy transitioning towards an elliptical morphology or a disk galaxy viewed at a high inclination. There's no evidence of strong tidal features or major disturbances, indicating the galaxy is likely not undergoing a major merging event, though a minor interaction cannot be ruled out. Overall, the galaxy exhibits characteristics of a moderately massive system with a moderate star formation rate.
