The galaxy presents as a relatively compact object. Its morphology is largely smooth, with a centrally concentrated luminosity profile. There are no clear spiral arms or a distinct disk structure evident. The core is bright and diffuse, with a rapid falloff in surface brightness moving outwards. The outer regions display some irregularities and faint extensions, especially towards the bottom left, hinting at possible tidal interactions or minor disturbances. The galaxy exhibits a blue hue, likely indicating the presence of a younger stellar population.
