The galaxy presents an overall elliptical morphology, though some asymmetrical features are apparent. The central region is dominated by a bright, concentrated bulge. The light distribution suggests an older stellar population, with a possible transition to a more extended, fainter halo. There is evidence of a faint disk-like structure around the core, although it appears somewhat disturbed or irregular. A notable feature is the apparent interaction or merging with a smaller, companion galaxy in the lower part of the image, exhibiting distinct tidal tails and morphological disruptions indicating an ongoing gravitational interaction. This disturbance suggests a minor merger event is occurring. The lack of prominent blue color suggests a lack of on-going active star formation.
