The galaxy presents a generally smooth morphology, appearing largely featureless at this resolution. It displays a concentrated central region with a gradual fading towards the outer edges. The shape is roughly elliptical, showing a slight deviation from perfect circularity. There are no clearly discernible spiral arms or bar structures visible. The color profile suggests a higher concentration of older stellar populations, particularly towards the core, implied by the yellowish hue. The outer regions show a slight bluer tint, indicating potentially younger stellar populations or ongoing, albeit minimal, star formation activity. There is no obvious evidence of significant tidal interactions or mergers with other galaxies. The galaxy appears to be relatively isolated and undisturbed, with its light distribution exhibiting a fairly regular and symmetrical profile.
