The galaxy presents as a somewhat elongated structure, exhibiting characteristics of a disk galaxy, though the disk appears inclined relative to our line of sight. Its color profile suggests a moderately active star-forming population, with the blue channel indicating the presence of hot, young stars within the galaxy, though not overwhelmingly so. The core appears relatively smooth and concentrated, with a diffuse halo. There is an absence of any clear spiral arm structure, suggesting either a smoother morphology or a possible distortion due to interactions. The redder regions suggest an older stellar population. There is a slight asymmetry in the galaxy's profile, with a more extended and slightly disturbed structure on one side, which may suggest a minor tidal interaction or merger event in its past. Overall, the galaxy appears to be a transitioning between disk and elliptical morphologies, with intermediate mass, and star formation rate.
