The galaxy appears to be a disk galaxy, viewed at a considerable angle, though not perfectly edge-on. There's a bulge that exhibits a concentrated luminosity with a yellow hue in the central region, suggesting a population of older stars. Extending outwards from the bulge is a fainter disk. The disk shows some subtle structural features, but they are not highly defined, indicating a relatively smooth or featureless morphology. The absence of strong spiral arms or other distinct features within the disk could suggest a lower ongoing star formation rate, though some level of star formation is likely present. Based on color, we are likely seeing an older population of stars in the arms. There's no strong evidence of any ongoing major merging events or strong tidal distortions.