The galaxy presents as a somewhat elliptical structure, although displaying some irregularities suggestive of possible interactions or internal disturbances. The central region appears bright and concentrated, indicating a significant stellar population and potential activity, possibly related to an active galactic nucleus. There is a yellowish hue to the core, suggesting an older stellar population. The outer regions are less defined, with hints of spiral arm structures or tidal features extending outwards. These outer areas exhibit a bluer color, consistent with the presence of younger, hotter stars and ongoing star formation. The overall appearance implies a galaxy with a substantial mass and an intermediate level of star formation activity. There is a possible minor merger or interaction with a smaller object that has disrupted the disk shape, and increased the rate of star formation.
