The galaxy appears to be a relatively smooth, elliptical-shaped structure, elongated along its major axis. Its core region exhibits a brighter, yellowish hue, suggesting a higher concentration of older stars. Progressing outwards from the core, the color gradually transitions to a bluer tone, especially noticeable in the outer regions. These bluer regions may be indicative of younger stellar populations, perhaps associated with ongoing or recent star formation activity, albeit at a low rate. There is no substantial indication of any distinct spiral arm structure or prominent dust lanes. The galaxy seems generally undisturbed, with only minor hints of potential tidal features or distortions that would suggest a past or ongoing minor merger event. The galaxy presents a regular and mostly homogenous structure, with no clearly detectable signs of active galactic nuclei features.
