The galaxy presents an overall elliptical morphology, exhibiting a smooth, featureless structure in the available optical bands. The luminous profile is concentrated toward the center, with a noticeable radial decrease in surface brightness. The galaxy's major axis appears moderately elongated, with a suggestion of a mild disk component. The central region displays a yellowish hue, possibly indicating an older stellar population and a relatively low rate of ongoing star formation. The outskirts of the galaxy show a subtle blue tint, hinting at the presence of younger, hotter stars, though the rate of star formation is subdued. There is no evidence of significant tidal disturbances or major mergers. The galaxy does not show any pronounced spiral arm structures or prominent dust lanes.
