The galaxy appears as a moderately luminous object with an overall concentrated profile. It exhibits a relatively smooth morphology, though some irregularities and features are present.

The galaxy's central region presents a bright, slightly yellowish core, indicating the presence of an older stellar population. A faint, extended disk or halo surrounds the core, displaying a bluer hue, possibly suggesting younger stars or ongoing star formation. Patches of redder regions can be discerned throughout the galaxy, potentially indicating areas of dust obscuration or older stellar populations. There is some evidence of a slight disturbance in the shape of the galaxy with some suggestions of an interaction or minor merger, although a single, dominant body is still quite apparent.
