The galaxy presents a moderately elongated morphology, appearing as an intermediate form between a disk and a spheroidal shape. The central region exhibits a smoother texture, potentially indicating a bulge component. Hints of a disk structure are suggested by the subtle extension along the major axis, though any spiral arms, if present, are not clearly resolved in this image. The color profile suggests the presence of both older stellar populations, indicated by the reddish hues, and regions of more recent star formation activity, revealed by the bluer tones, distributed throughout the galaxy. There are hints of minor disturbances in the galaxy's morphology, possibly due to past or ongoing interactions.
