This galaxy presents as a moderately bright object with an apparent morphology that tends toward elliptical. The central region exhibits a high degree of surface brightness, appearing almost uniformly luminous in the available data. Moving outwards from the center, there's a notable, albeit faint, ring-like structure, indicating a potential feature or structure in its distribution of stars, dust, or gas. This outer ring is not uniformly colored. There is evidence of subtle disturbance in the overall structure. The galaxy shows a slight distortion of the overall symmetry, hinting at a possible interaction or minor merger event in its past or present. The color distribution suggests a relatively smooth transition, although there are some mottled areas which could be indicators of star-forming regions or differing stellar populations.
