The galaxy presents an elongated, spindle-like morphology. It exhibits a smooth, centralized luminosity profile, indicative of a large population of older stars. The core is a concentrated yellow, surrounded by a less concentrated white light. There is no strong evidence of spiral arm structures, suggesting that the galaxy is most likely an elliptical or lenticular galaxy. While a slight asymmetry is present, there is no prominent sign of tidal disturbances or interactions with other galaxies. Star formation appears to be suppressed.
