The galaxy appears to be an elliptical galaxy, exhibiting a smooth, diffuse structure with no prominent spiral arms or distinct features. The light distribution suggests a centrally concentrated bulge. It has an elongated, cigar-like shape, with the major axis extending approximately twice as long as the minor axis. A color gradient is subtly present, trending from slightly bluer hues towards the outer regions to warmer, redder tones at the core. This color variation suggests a possible difference in stellar populations, with older, redder stars concentrated in the central bulge and a younger, bluer population at the edges. There is no discernible dust lane or recent star formation.
