The galaxy presents a generally smooth morphology, appearing largely featureless at this resolution. Its shape approximates a rounded form, though it is neither perfectly circular nor significantly elongated. The dominant color is a yellowish-orange hue, which is indicative of a stellar population that is largely comprised of older, less massive stars. This suggests a relatively low rate of ongoing star formation. The galaxy's size is relatively compact, and no distinct spiral arms or a prominent central bulge are discernible. The light is centrally concentrated, which reinforces the conclusion that the galaxy is dominated by older stellar populations and lacks the patchy structure associated with active star-forming regions. There is no evidence of tidal tails or other distortions that would indicate a recent or ongoing merger event.
