The galaxy presents as a centrally concentrated, roughly elliptical object. The core exhibits a bright, yellowish-white luminosity, suggesting an older stellar population is dominant there. Moving outward from the core, the light becomes less intense. A subtle color gradient is observed, with the outer regions displaying a slightly redder hue, indicative of potentially cooler or dustier regions further from the core. There are hints of faint, diffuse extensions, but no clear spiral arm structures or prominent features. Overall, the galaxy appears to be in a relatively relaxed state, lacking any major disturbances.
