The galaxy presents as a relatively smooth, centrally concentrated object with a notable lack of distinct spiral arm structure. Its overall shape appears somewhat elliptical, being neither perfectly spherical nor highly elongated. The color profile exhibits a yellowish-white hue towards the core, suggesting a population of older stars dominating the central regions. The light intensity diminishes gradually outwards, with a subtle transition to fainter, bluer tones in the outer regions, potentially indicating some presence of younger stellar populations. There is no obvious evidence of active galactic nuclei activity or significant dust lanes obscuring the galactic center. The galaxy does not appear to be undergoing any major merging events or showing signs of significant tidal disturbances. Minor irregularities are not clearly visible. 
