The galaxy presents a generally smooth morphology, appearing as a single, relatively homogenous luminous structure. Its shape is largely circular in projection, exhibiting minimal elongation or distortion. There is a slight change in color towards the center of the galaxy, suggesting the core is likely more metal-rich. The stellar population appears to be dominated by older stars, based on the redder color, although there might be some on-going, but low-level, star formation in the outer regions as suggested by the bluer light. There is no distinct nucleus or spiral arm structure visible. No signs of tidal interactions or ongoing mergers are observed, and the overall structure is quite regular and undisturbed.
