The galaxy exhibits a generally smooth morphology. It appears elliptical, with a notable elongation along its major axis. The central region is characterized by a bright, concentrated core, exhibiting a yellowish-white hue, suggestive of an older stellar population. Moving outwards from the core, a subtle gradient to a bluer color is observed, particularly at the edges of the galaxy, hinting at regions of possible recent star formation. There's no strong evidence of spiral arm structures or significant dust lanes within the image. The overall appearance points to a relatively evolved galaxy with a dominant smooth component, potentially undergoing limited current star formation. There are some irregular features that suggests that this may be a merger.