The galaxy appears as a singular, relatively smooth object with minimal visible structure. The overall shape is neither perfectly round nor elongated, appearing somewhat in-between. There is no clear evidence of spiral arms or a distinct central bulge. There is no apparent merging activity or major disturbances. The light is fairly concentrated, giving the galaxy a somewhat compact appearance. The galaxy displays a slightly bluish hue, which may suggest the presence of young, hot stars and ongoing star formation, although the rate of star formation appears relatively low.
