The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a concentrated, bright core that transitions smoothly into a more diffuse outer region. The overall shape leans towards round, but exhibits a moderate ellipticity.

The color profile is dominated by warmer tones, suggesting a population of older stars. There's a noticeable absence of prominent blue colors typically associated with active star formation. No distinct spiral arms or bar structures are evident. There are no obvious signs of major disturbances or mergers, although some subtle irregularities in the outer regions cannot be entirely ruled out.
