This galaxy appears to be a spiral galaxy with a prominent central bulge. The bulge exhibits a yellowish hue, suggesting a population of older stars. The disk component appears fairly well-defined, but the spiral arms are not particularly tightly wound. The galaxy displays an intermediate inclination angle relative to our line of sight. Some clumpy structures are present within the disk, potentially indicative of star forming regions. The spiral arms appear relatively symmetric, with a possible weak bar structure in the center. No major signs of significant tidal interactions or mergers with other galaxies are immediately apparent.