The galaxy presents as a moderately sized elliptical, approximately 4.5 kpc in radius. It appears largely featureless, with a smooth light distribution, displaying a concentrated central bulge. The light is predominantly redder in the core, with bluer hues appearing in the outer regions, suggesting a mix of stellar populations with older stars more concentrated in the central region. The galaxy does not seem to be perfectly symmetrical. There is a slight elongation visible, with an approximate b/a ratio of 0.7, indicating a mild flattening. There is no clear evidence of spiral arms or dust lanes, and the morphology indicates it has not experienced a recent major merger, though some minor disturbance cannot be ruled out given the asymmetry. The Sersic index is around 1, suggesting it is close to an exponential profile.
