The galaxy presents an elongated, possibly cigar-shaped morphology. A prominent central bulge is visible, exhibiting a smooth, relatively featureless appearance. Faint blue features are observed, suggesting some ongoing star formation, likely within the disk component. The disk itself shows a subtle inclination relative to our line of sight. There appears to be some indication of minor disturbances, possibly suggesting past or ongoing gravitational interactions. Evidence of merging or major disturbance is subtle. Overall, the galaxy appears to be an intermediate-mass spiral galaxy, with a moderately low star formation rate.
