The galaxy presents an overall elliptical morphology, exhibiting a centrally concentrated luminosity profile. A smooth, featureless structure dominates, with a noticeable lack of distinct spiral arms or bar structures. The central region displays a bright, yellowish hue suggestive of an older stellar population. Moving outward from the center, the color transitions subtly to a bluer shade, hinting at the presence of a younger stellar population in the galaxy's outer regions. The galaxy appears elongated, departing from a perfectly circular shape. There is no apparent evidence of ongoing major mergers or significant tidal disturbances in the galaxy's immediate vicinity. Faint, diffuse features are possibly present in the outer halo, but a high degree of certainty is not possible given the image resolution.
