The galaxy presents as a roughly elliptical structure with a brighter, more concentrated central region. There is a discernible disk component, exhibiting a slightly elongated shape. The color profile is dominated by bluish hues, suggesting the presence of relatively young stars, likely indicative of ongoing or recent star formation, although at a very low rate. The galaxy exhibits signs of morphological disturbance, hinting at possible gravitational interactions with another galaxy or past merger events. The outer regions of the galaxy appear somewhat diffuse, lacking well-defined boundaries. A weak tidal feature may be present, further supporting the possibility of past or ongoing interactions.
