This galaxy presents a predominantly smooth morphology with a slight elongation. Its color profile suggests a relatively mature stellar population, indicated by the central region exhibiting a yellowish hue. Faint, bluer regions are observed at the edges, hinting at ongoing or recent star formation within the disk or spiral arms. The lack of distinct spiral arm structures or a prominent bulge points towards a possible intermediate disk system or a transition towards a more elliptical galaxy type. There is no strong evidence of major merger activity, although subtle asymmetrical features suggest minor gravitational interactions may be present.
