The galaxy presents as a single, largely homogenous structure. The light distribution appears smooth and centrally concentrated, exhibiting a near-spherical morphology. There is no apparent spiral arm structure or distinct disk component visible. The galaxy has a yellowish hue, suggesting an older stellar population and/or a relatively low rate of on-going star formation. There is no indication of any major mergers or significant tidal disturbances. The light profile gradually fades with increasing distance from the galactic center.
