This galaxy appears to be a spiral galaxy, although its features are somewhat blurred, possibly due to distance and/or resolution limits. The galaxy presents as elongated along a major axis. A bright central bulge is prominent and exhibits a yellowish-white hue, indicative of an older stellar population. Extending outwards from the bulge, fainter, bluish regions suggest the presence of spiral arms, which are tightly wound. These areas likely contain younger, hotter stars and ongoing star formation. There does not appear to be significant distortion or tidal features, implying a relatively undisturbed system without recent major merger events. The overall structure suggests a disk galaxy viewed at a significant inclination. The galaxy exhibits an estimated effective radius of approximately 4 kpc. Based on its color, the galaxy is thought to be on the more massive side and has an estimated ongoing star formation rate.
