The galaxy presents as a centrally concentrated spheroid of moderate angular size. The core region exhibits a high surface brightness, appearing almost unresolved in the available imaging. Surrounding the core is an extended envelope of fainter, more diffuse light. There is some evidence of subtle structural features, possibly indicative of a disk component, though the spheroid dominates the overall morphology. The galaxy's color appears relatively uniform across its extent, suggesting a consistent stellar population. The galaxy shows no indications of strong tidal disturbances or ongoing major mergers, but a very slight irregularity could indicate a minor interaction. The overall form is somewhere between a perfect sphere and a cigar shape.
