The galaxy exhibits a generally elliptical morphology, appearing largely smooth and featureless at this resolution. The central region is characterized by a bright, concentrated core that gradually fades into the outer regions. There is little evidence of distinct spiral arms or significant dust lanes. The color profile suggests a higher concentration of older stellar populations, trending towards redder hues, with a gradual shift towards bluer tones in the fainter outer regions. The overall color distribution is relatively uniform. The galaxy displays a slight elongation.
