The object appears to be a relatively small galaxy, exhibiting a roughly elliptical morphology with a diffuse structure. The light distribution suggests a central concentration, but without a clearly defined nucleus or bulge. The overall color is bluish, indicating a population of relatively young, hot stars and ongoing star formation within the galaxy. There is some evidence of spiral arm structure, but it is poorly defined. No bar structure is visible. The galaxy shows signs of disturbance, possibly from a minor merger or gravitational interaction.