The galaxy appears to be a spiral galaxy, viewed at a slight angle. It exhibits a prominent central bulge, which is approximately yellowish in color, suggesting an older stellar population. Extending from the bulge are two well-defined spiral arms, displaying a moderate winding pattern. The arms appear somewhat clumpy, indicating regions of active star formation. The disk component shows a complex distribution of color, with some regions showing bluish tints indicative of younger stars and others tending towards a more reddish hue. The overall structure suggests a barred spiral morphology, with a strong central bar-like feature evident. There is no visual evidence of major mergers or tidal disturbances, though some faint asymmetry in the spiral arm structure cannot be ruled out as a minor interaction.
