The galaxy presents a generally smooth, elliptical morphology with a relatively high degree of central concentration.  The core region exhibits a redder hue, suggesting a population of older stars and/or a significant dust component. The outer regions appear less centrally concentrated and show a gradual color shift towards bluer hues, which indicates the presence of younger stellar populations. There is no evidence of strong spiral arm structures or a prominent disk component. The galaxy's overall shape appears closer to round, with only slight elongation. There's no clear visual evidence of on-going major merging activity, however, there may be minor disturbances.