This galaxy exhibits a generally elongated, cigar-like morphology. The central region displays a higher concentration of light, appearing yellowish in color, suggesting an older stellar population. Extending outward from the core are fainter, bluer regions. The overall structure appears to be relatively undisturbed, with no obvious signs of recent major merger events. However, there is a slight asymmetry and some evidence for minor disturbances in the outer disk, possibly indicating past or ongoing interactions. The galaxy's disk is seen at a high inclination, which contributes to its elongated shape. Star formation appears to be ongoing, as indicated by the bluer regions in the disk, but at a relatively low rate. The galaxy is estimated to be of intermediate mass.
