The galaxy appears as a centrally concentrated object with a generally smooth morphology. Its overall shape is elliptical, with a noticeable but not drastic elongation. The core exhibits a bright, concentrated luminosity, indicating a high density of stars in the galactic nucleus. The color profile suggests a presence of older stellar populations, with a subtly redder hue in the outer regions compared to the bluer, brighter central core, which may imply ongoing or recent star formation activity. There are no prominent spiral arms or dust lanes visible. Faint, diffuse light extends outwards from the core, gradually fading into the background. No significant tidal features or interactions with other galaxies are apparent in this field. The overall appearance suggests a relatively evolved galaxy.
