The galaxy presents as a single, relatively smooth object with a concentrated central bulge. Its overall morphology appears elliptical, exhibiting a slight elongation without any prominent spiral arm structures or significant disk features visible in the image. The color gradient suggests a higher concentration of older stellar populations within the central bulge, which exhibits a yellowish hue. Moving outwards from the core, the color appears to subtly shift towards redder tones. No obvious tidal tails, dust lanes, or ongoing major mergers are evident. There is a hint of a slight asymmetry, possibly indicating a minor interaction or recent accretion event, though further investigation would be required to confirm this. The overall smoothness points to the likelihood that this galaxy is a relatively evolved system.
