The galaxy presents as a somewhat centrally concentrated object with a noticeable smooth morphology, though it is difficult to assess fine details at this resolution. The core exhibits a pronounced brightness, suggesting a high density of stars or possibly an active galactic nucleus, but this is unclear. The light distribution appears relatively even, without strong evidence of spiral arms or distinct morphological features. The galaxy displays a slight elongation, but it is largely rounded in appearance. There are hints of faint, diffuse extensions surrounding the main body of the galaxy, but these are indistinct. There does not appear to be any significant interaction with nearby galaxies, nor significant disruptions to its structure. A color gradient is visible, with the core exhibiting a yellower hue that transitions to slightly bluer tones in the outer regions, which could indicate different stellar populations.
