The galaxy appears to be a spiral galaxy at an estimated distance corresponding to a redshift of approximately 0.06. Its morphology leans toward a disk-like structure with features suggesting a spiral arm presence, although the spiral arms are not well-defined and are somewhat flocculent. There is a noticeable central bulge, exhibiting a bright and concentrated luminosity profile. The galaxy's overall color is intermediate, with a yellow hue to the core that shifts towards blue in the outer regions. The color gradient implies the likelihood of ongoing star formation, particularly in the outer regions. Based on the color, the average metallicity is likely to be high, though there are signs of some degree of disturbance to the overall structure that may imply some past merger or interaction.
