The galaxy presents as a concentrated, centrally-brightened system. Its light profile appears relatively smooth, with no immediately obvious spiral arm structures or prominent dust lanes visible at this resolution. The overall shape is generally elliptical, tending towards a more circular morphology. There is a very slight elongation. The central core is a yellowish hue, suggesting an older stellar population or significant dust obscuration. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances based on its morphology; it presents as a relatively relaxed system.
