The galaxy presents as a spiral type, exhibiting a distinct disk structure viewed at a slight angle, but mostly face-on. The central bulge appears moderately sized and exhibits a yellowish hue, suggesting a population of older stars. Two prominent spiral arms are visible, characterized by a relatively medium winding pattern. Star formation appears active within these arms, indicated by the presence of bluer regions. There is some indication of a bar-like structure extending from the bulge, though not particularly pronounced. There may be some signs of minor disturbances or interactions, but they are not overly drastic. The overall structure is well-defined, and the galaxy appears relatively isolated.