This galaxy presents a generally smooth morphology, though subtle features are discernible. The primary body of the galaxy exhibits an elongated, cigar-like shape. A brighter, more compact region is observed at one end, possibly indicating a concentration of stellar material or an active galactic nucleus. A diffuse, extended halo appears to emanate from the main body, gradually fading into the background. There is some indication of minor disturbance of this shape in the form of uneven lighting. This may be an indication of minor merger activity or internal dynamic processes within the galaxy. The overall color profile suggests a population of older stars, with a warmer central glow that shifts toward slightly bluer tones in some of the outer regions.
