The galaxy presents as a moderately luminous object with an overall yellowish hue, suggestive of a stellar population dominated by older stars. The morphology appears to be intermediate between a smooth, elliptical galaxy and a disk galaxy with some features. There is a central, brighter region, possibly a bulge or a concentration of older stars. Hints of a disk-like structure can be observed surrounding this central region, however the arms are not clearly defined. The apparent shape of the galaxy appears distorted, possibly indicating ongoing or past interaction with another galaxy. There is a suggestion of minor tidal disturbances and/or merger activity influencing its structure.
