The galaxy presents as a relatively smooth object with some discernible features. The central region exhibits a bright, concentrated core, suggesting a significant population of older stars. Moving outwards from the core, the light gradually diminishes into a less defined disk or envelope. There are subtle indications of spiral arm structures or disk-like features, though these are not sharply defined. These outer regions show a bluer hue compared to the core, suggesting the presence of younger, hotter stars and ongoing star formation, but the rate appears moderate. The overall shape is somewhat elongated, appearing between round and cigar-shaped and indicating a potential elliptical or lenticular morphology seen at an angle, but the presence of star formation indicates it is more likely a spiral galaxy. There is a slight asymmetry in the outer regions, suggesting a possible minor disturbance or interaction event.
