The galaxy presents a largely smooth and rounded morphology, suggesting it may be of elliptical type, or perhaps a spiral seen face-on. The light is concentrated towards the center with a distinct bulge. Faint, diffuse edges are visible, gradually fading into the background. The galaxy exhibits a yellowish-orange hue, which might indicate an older stellar population with a lower rate of star formation and dust content. A subtle colour gradient is visible, transitioning from yellow-orange in the center to a more reddish colour towards the outer parts. There are no prominent spiral arm structures or significant dust lanes visible in this image. There is a slight irregularity towards the top of the galaxy, perhaps indicating the presence of some type of minor interaction. Overall, the galaxy appears to be a fairly relaxed system with limited ongoing star formation.
