The galaxy exhibits an overall smooth morphology, potentially exhibiting some disklike features. Its shape appears largely rounded, deviating slightly from a perfectly circular form and leaning toward a more elongated, albeit not significantly cigar-shaped, structure.

There is a slight asymmetry, where one edge of the galaxy appears to be slightly more extended than the other, suggesting the possibility of minor tidal interactions. The core of the galaxy shows a concentrated, bright emission, indicative of either a dense stellar population or possible activity from a supermassive black hole.

Color gradients are visible throughout the galaxy. The central region has a yellow/white hue, possibly suggesting a population of older stars. The outer regions exhibit a slight blue tinge, potentially indicating the presence of younger, hotter stars, hinting towards ongoing star formation.
