The galaxy appears as a centrally concentrated object, with a generally smooth morphology. The color profile suggests a dominant population of older stars, indicated by its redder hue. There is no apparent spiral structure or significant dust lane obscuration visible in this image. The object displays a high degree of circular symmetry, with minimal elongation. Evidence of tidal features or merging activity is absent, suggesting it is an undisturbed system. The overall luminosity profile indicates a relatively passive galaxy, likely with a suppressed star formation rate. Its size suggests a galaxy of considerable mass.
