The galaxy appears as a centrally concentrated object with a generally smooth morphology. The light profile suggests a dominant bulge component, with a gradual decline in surface brightness from the core outwards. There's a hint of an extended halo, though its faintness makes detailed characterization difficult. The galaxy appears slightly elongated. The overall color is relatively uniform, with a reddish-yellow hue, indicative of an older stellar population and/or significant dust extinction. There is no clear evidence of strong spiral arms or prominent star-forming regions. Any features indicative of a recent major merger event are absent, with minimal signs of tidal disruption or asymmetry.
