The galaxy appears as a flattened, disk-like structure, viewed at a high inclination. The central region exhibits a yellowish hue, suggesting an older stellar population likely concentrated in a bulge. Progressing outwards from the center, a bluish tint becomes more apparent, indicative of younger, hotter stars potentially within spiral arms. These arms are not well-defined, appearing somewhat patchy and diffuse. The overall smooth texture of the galaxy implies a relatively evolved system, without significant ongoing major merger events. There may be minor disturbances or tidal features, although the image resolution limits definitive identification. The galaxy's size, while moderate, suggests a substantial stellar mass, placing it as potentially a late-type spiral galaxy. Star formation is ongoing but does not appear to be dominated by intense, localized events.