The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears to be an intermediate form between elliptical and disk galaxies. There is a bright, well-defined central bulge with a yellowish hue, indicating a population of older stars. The galaxy exhibits a slight elongation, appearing more oval than perfectly spherical. A faint disk component is visible surrounding the bulge, but it lacks prominent spiral arm structures. The colors transition gradually from the yellowish core to a bluer outer region, suggesting the presence of some younger stars and ongoing, but perhaps subdued, star formation within the disk. There are no obvious signs of a major ongoing merger, although minor tidal disturbances cannot be completely ruled out based on this image alone. Overall, the galaxy seems to be a moderately massive system, transitioning from a more actively star-forming stage to a more quiescent state dominated by older stellar populations.
