The galaxy presents a generally smooth morphology. The light distribution suggests an elliptical or lenticular (S0) classification, characterized by a lack of distinct spiral arms. The galaxy is roughly elliptical in shape but appears to have a slight disk-like structure. The core of the galaxy exhibits a bright, concentrated region indicative of a high density of stars. The color appears to be relatively uniform, trending toward the redder end of the spectrum. It shows a smooth falloff in luminosity from the core to the outer regions. There is an apparent flattening, and a somewhat cigar shape is observed. No signs of active galactic nuclei or recent merger activity can be seen in this image.
