The galaxy presents as an elliptical morphology, exhibiting a somewhat elongated shape. The light profile appears smooth and centrally concentrated, with a gradual decrease in intensity towards the outer regions. The central region displays a yellowish hue, potentially indicating an older stellar population. Fainter, diffuse blue light extends beyond the central bulge, perhaps suggesting the presence of some younger stars or ongoing star formation within the extended disk. A subtle asymmetry in the outer regions may hint at minor tidal interactions or past mergers. The galaxy's structure is generally well-defined, lacking obvious prominent features such as spiral arms or strong dust lanes.
