The galaxy appears to be a relatively smooth, elliptical system. Its morphology is primarily spheroidal, exhibiting a concentrated central bulge which gradually diffuses outwards. The light profile suggests a redder stellar population, indicative of an older stellar age, particularly within the central regions. The ellipticity is moderate, leaning towards an 'in between' shape; it is neither perfectly spherical nor highly elongated. There is little evidence of distinct spiral arm structures or prominent dust lanes. A faint halo may be present, extending beyond the main body, though this is difficult to ascertain due to the limitations in image resolution. Overall, the galaxy appears to be a quiescent, relatively undisturbed system. There are no signs of any merging activity or interactions with nearby objects.
