The galaxy exhibits a generally smooth morphology, appearing largely featureless in the image. It appears to have a somewhat round shape. A concentrated central region is visible, suggestive of a bulge. The galaxy presents a relatively uniform color gradient from the center outwards. The light emitted is bluer in the central region, indicating higher star formation activity and/or the presence of younger stellar populations there, and shifting slightly toward redder hues further out, suggesting older stellar populations in the outer regions. There does not appear to be evidence of strong tidal interactions or major disturbances in the galaxy's structure, nor are spiral arms apparent.
