The galaxy presents as a centrally concentrated object with a smooth, largely featureless morphology. The light distribution suggests an elliptical or lenticular classification, showing minimal evidence of spiral arms or prominent dust lanes. The galaxy exhibits a yellowish-red hue, indicating a stellar population dominated by older, redder stars, suggesting lower levels of recent star formation. The object appears relatively isolated, with no obvious signs of tidal disturbances or ongoing mergers, though a faint area to the lower left indicates a possible minor gravitational interaction. Overall, the galaxy gives the impression of being a relatively evolved system with a substantial stellar mass.
