The galaxy presents as a moderately sized, luminous structure with an overall elliptical morphology. The light distribution appears relatively smooth and centrally concentrated, suggesting an older stellar population. There is a subtle but notable deviation from perfect ellipticity, potentially indicating minor disturbances or interactions with other galaxies or ongoing internal processes, such as minor mergers. There's a hint of a disk-like feature although faint. The color profile is suggestive of a galaxy with a dominant population of evolved stars.
