The galaxy presents as a single, relatively smooth object. Its overall shape is generally elliptical, exhibiting a moderately rounded morphology. There is a slight elongation to the structure, but it isn't highly pronounced. The central region appears brighter and more concentrated, suggesting a higher density of stars or the presence of an active galactic nucleus. The color distribution is somewhat uneven. The central core exhibits a yellowish hue, possibly indicative of an older stellar population. Extending from the central region, there are indications of subtle disturbances or tidal features, potentially related to a minor interaction or past merger event. The outer regions appear fainter and bluer, suggesting a population of younger stars. There are indications of ongoing star formation. Although the galaxy seems relatively isolated, there is evidence of potential interactions or disturbances within its structure, hinting at a more complex history.
