The galaxy appears as a centrally concentrated object with a generally smooth morphology. The light profile suggests a centrally dominant spheroid, possibly an elliptical galaxy or a lenticular galaxy seen at an oblique angle. There is a slight elongation to the galaxy's shape, with a round to in-between classification. The colour is a relatively even yellow-orange hue, suggesting an older stellar population with lower levels of current star formation activity. No distinct spiral arms or prominent dust lanes are visible. There is little indication of any major merging activity or tidal disturbances based on the galaxy's overall structure.
