The galaxy appears as a centrally concentrated object with a generally smooth morphology. There is evidence of a slight elongation, suggesting it is not perfectly spherical. The color profile indicates a dominant population of older stars, seen as the yellowish-red hue. The galaxy lacks the distinct spiral arms or significant dust lanes typically seen in late-type spiral galaxies. The light is centrally condensed with decreasing intensity towards the edges. Faint features or disturbances are not readily apparent, but some subtle irregularities in the outer regions suggest potential past interactions.
