This galaxy exhibits a centrally concentrated morphology, appearing generally smooth with a slight elongation. The core presents a bright, compact structure. Moving outwards, the luminosity gradually decreases, transitioning into a fainter, more diffuse outer region. The galaxy displays a subtle disk-like appearance with no clear spiral arm structure. A marginal level of disturbance may be present, potentially indicating a minor interaction or internal asymmetry. The overall color profile suggests a relatively evolved stellar population with a moderate rate of star formation. The estimated physical size is approximately 6 kpc in radius.
