The galaxy presents as a relatively small, face-on or nearly face-on system, exhibiting a generally elliptical morphology. The light distribution suggests a centrally concentrated bulge, surrounded by a fainter, more diffuse halo. The core appears to be fairly bright, with an overall blue hue, suggesting relatively recent or ongoing star formation. The outskirts of the galaxy fade gradually into the background, making it hard to discern whether the halo is even or disrupted in any way. There is no obvious spiral arm structure visible. The object seems largely undisturbed, with no apparent signs of a major ongoing merger, although a minor tidal interaction cannot be ruled out based on the available imagery.
