This galaxy presents a relatively smooth morphology, with an overall elongated, cigar-shaped appearance. The central region exhibits a concentrated, bright core with a yellowish hue, suggesting an older stellar population. Fainter, bluer light is detected in the surrounding areas, indicating the presence of younger stars or ongoing star formation. There is no obvious spiral structure visible. No signs of recent major mergers are seen, although the light is somewhat disturbed, possibly indicating a minor interaction or internal dynamic processes. The galaxy is observed at a redshift of approximately 0.29, and a physical scale of around 10 kpc. This puts the galaxy at a significant distance, with an estimated mass and relatively high star formation rate.
