The galaxy presents as an elongated, cigar-shaped structure, potentially an elliptical galaxy viewed at an oblique angle or a highly inclined spiral. The light distribution is relatively smooth, with a noticeable color gradient. The central region appears to be more luminous and exhibits a yellowish hue, suggesting an older stellar population, which is consistent with it being elliptical. Fainter, bluish emission, possibly indicative of younger stars or active star formation, is present. There may be evidence of minor tidal disturbances, but this requires further investigation at higher resolution. The overall morphology does not suggest a major ongoing merger, but minor interactions cannot be ruled out without more detailed spectral and spatial information. The estimated size indicates a relatively large galaxy.