The galaxy presents a generally smooth and rounded morphology. Its light distribution appears concentrated, with a noticeable central bulge. There are no distinct spiral arms or bar structures discernible. The overall color profile appears to be dominated by yellowish-red hues, suggesting an older stellar population. Subtle variations in color exist within the galaxy, showing a green hue at the edges and a slightly more blueish-purple tint in the center. The galaxy is fairly isolated, showing no obvious signs of tidal interaction or ongoing major merger events.
