The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is circular with an average radius of approximately 4.3 kpc. Color gradients within the galaxy are subtle, with a slight blue-ish hue across the entire galaxy suggesting the presence of at least some on going star formation. A faint disc is visible through the color gradient of the galaxy, however further analysis is required to asses the details of its shape and any spiral structure that may be present. No major signs of tidal disturbance or ongoing merger activity are immediately apparent. The light distribution appears centrally peaked, hinting at the possible presence of a supermassive black hole, however additional data and analysis will be needed to make any conclusions.
