The galaxy presents a generally smooth morphology. The light is centrally concentrated, with a core region exhibiting a yellowish hue, suggesting an older stellar population. The overall shape appears close to round with a slight deviation towards an intermediate elliptical form. There is no apparent evidence of a prominent disk, spiral arms, or significant dust lanes. There is no indication of ongoing or recent major merging activity or tidal disturbances. The lack of bluer colors suggests a relatively low current star formation rate.
