The galaxy presents a generally smooth morphology with a slight asymmetry in its outer regions. The central bulge is prominent and exhibits a concentrated luminosity, suggesting a high stellar density in this region. The color gradient transitions from a yellow-orange core to a redder hue in the outer disk or halo, potentially indicating differences in stellar populations or dust content. The overall shape appears elliptical, with no obvious spiral arm structures visible. There is a minor indication of disturbance in the galaxy’s profile, however this is subtle and may not be a significant morphological aspect.
