The galaxy presents a generally elliptical morphology, though not perfectly spherical. There is evidence of a slight flattening. The galaxy exhibits a relatively smooth texture with no distinct spiral arms or bars visible. A faint, diffuse halo seems to surround the central, brighter region. The color appears bluish, suggesting the presence of younger stars and ongoing star formation within the galaxy. There may be some level of disturbance from either a smaller merger or some other gravitational interaction.
