The galaxy exhibits a relatively smooth morphology, with a central bulge that appears predominantly yellow. The color suggests a population of older stars. Moving outward from the bulge, the disk component displays a slightly bluer hue, indicative of ongoing or recent star formation. However, spiral arm structures are not clearly defined. There are some slight asymmetries observed in the galaxy's outer regions, potentially signifying minor gravitational interactions or internal disturbances. Overall, the galaxy presents as having intermediate luminosity and a mass comparable to typical spiral galaxies. The estimated star formation rate implies moderate levels of stellar birth activity. The overall structure shows a round shape, typical of a galaxy with a dominant bulge.
