The galaxy presents with an overall smooth morphology. The light distribution appears centrally concentrated and somewhat spheroidal. There is an indication of a possible secondary concentration of light situated toward the left, suggesting a mild disturbance or interaction. A color gradient is visible across the galaxy, with the right side appearing bluer and the left side exhibiting a more yellow-red hue. The redder hue suggests an older stellar population, possibly with more dust obscuration. The bluer region is indicative of younger, hotter stars or less dust obscuration. A very minor, subtle elongation is hinted at but the form appears close to spherical.
