This galaxy presents as a moderately faint, somewhat diffuse object. It appears to possess both a spheroidal component and a disk-like component. The spheroidal component has a slightly brighter core, indicative of a higher concentration of stars in the galactic center. The disk is visible extending outwards from the central region. The galaxy exhibits a blue hue, particularly in the outer regions, potentially indicating ongoing star formation. There appears to be some visual indication of disturbance in the structure, but nothing too disruptive. This could potentially be attributed to a minor merger event, or some internal process occurring in the galaxy.
