The galaxy presents a generally smooth, rounded morphology with an apparent moderate size. The dominant color is bluish-white, suggesting a relatively high population of young, hot stars and ongoing star formation. A bright, concentrated central region is visible, possibly indicating the presence of an active galactic nucleus or a dense stellar population. There is some visual evidence of minor disturbances or features in the outer regions, such as slight irregularities or extensions, which could point to tidal interactions or past merger events.
