The galaxy presents as a luminous, yellowish-white object with an approximate radius of 5 kpc. It appears to have a relatively smooth morphology, suggesting a lack of prominent spiral arms or distinct features. The light distribution exhibits a centrally concentrated profile, with the intensity decreasing gradually towards the outer regions. The overall shape is close to circular. There is some evidence of minor disturbance within the galaxy, along with a small region showing a reddish tint possibly caused by dust absorption or a population of older stars. The galaxy also shows evidence of being in a merger or tidal interaction.