This galaxy presents as an elongated, cigar-shaped object. The core region exhibits a concentrated, bright profile with a yellowish-orange hue. The color suggests a potential aging stellar population within the bulge. The luminosity decreases gradually moving outward from the center, fading into the background. There is some structural disturbance; a slight asymmetry is observed in the outer regions. Hints of bluer tones can be detected on the edges, suggesting the presence of ongoing star formation, albeit at a modest rate. The lack of distinct spiral arms points toward an evolved disk or perhaps a transitioning morphology. The object doesn't present any significant signs of a major merger event.
