The galaxy presents as a spiral type, observed at an inclined angle relative to our line of sight. The disk component is prominent, with spiral arms clearly visible though somewhat tightly wound. A central bulge is apparent, displaying a yellowish hue, which indicates an older stellar population likely located at the center. The spiral arms are bluer in color, suggesting ongoing star formation activity, and appear relatively well-defined. Indications of a possible bar structure are present, though it does not appear to be a strong or defining feature. The overall structure seems largely undisturbed, with no significant signs of recent major mergers or tidal disruptions. The galaxy exhibits a moderate degree of central concentration of light, gradually fading outwards into the disk.
