The galaxy appears to be composed of two distinct, somewhat diffuse luminous regions. The brighter of the two is more extended and appears nearly circular. The second, smaller region, sits below and to the left and appears to be a separate condensation of light. The overall morphology suggests that the object may be undergoing a minor interaction or merging event, resulting in some disturbance of its overall structure. A notable portion of light could be attributed to artifacts, potentially impacting the assessment of the galaxy's true structure and morphology. The galaxy's shape is mostly round, with some indication of a departure from perfect circularity and a slight deviation toward a cigar shape. This shape might support the notion of a system undergoing some kind of dynamic process.
