The galaxy presents as a relatively compact object with a generally smooth morphology. There appears to be a central bulge that dominates the overall light profile. The galaxy appears flattened, but not to the degree seen in edge-on disk galaxies. There is faint evidence of a disk component or spiral arms. The color profile suggests a mix of stellar populations; bluer colors are evident in the outer regions, perhaps indicative of ongoing star formation, while the central bulge exhibits a yellower hue, consistent with older, redder stars. There is no apparent major merger activity occurring, however, it may be undergoing a minor interaction. The is no prominent dust lane evident within the galaxy.