The galaxy presents as a centrally concentrated object with a generally smooth morphology. Its overall shape appears somewhat rounded, though not perfectly circular, exhibiting a mild degree of ellipticity. The color is dominated by orange hues, suggesting an older stellar population and a relative paucity of recent star formation. There is a subtle hint of asymmetry or disturbance in the outer regions, possibly indicative of a minor interaction or past merger event. The galaxy does not display a prominent disk or spiral arm structure in this imaging. There are a few regions of slightly enhanced red color in the vicinity of the galaxy, these could potentially be regions of high dust concentration or star formation.
