The galaxy appears to be an elliptical type, exhibiting a smooth, featureless morphology. It presents an elongated shape, more akin to a flattened spheroid than a perfect circle. The central region is brighter and more concentrated, suggesting a higher density of stars. The color profile indicates a predominantly older stellar population, displaying a redder hue in the outer regions transitioning to bluer wavelengths towards the nucleus, possibly indicative of more recent, albeit low, star formation activity in its core. There is no visible evidence of spiral arms, dust lanes, or active galactic nuclei-related jets. There is a potential faint distortion suggesting a possible past or ongoing minor merger event. The overall impression is that of a mature galaxy, likely having undergone significant evolution and exhibiting a relatively quiescent state.
