The galaxy presents a smooth, elliptical morphology. It exhibits a high degree of central concentration, with a bright, well-defined core that gradually fades outwards. There is a noticeable lack of distinct spiral arm structures or prominent dust lanes. The color profile appears relatively uniform, displaying a yellow-red hue characteristic of an older stellar population. No significant tidal features or signs of ongoing mergers are readily apparent. The overall appearance suggests a galaxy in a relatively quiescent state, potentially approaching a passive evolution phase.
