The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light profile appears to decrease gradually from the core outwards, with no obvious spiral arm features. It is oblong, exhibiting an apparent flattening. The galaxy's color profile indicates a dominant population of older stars, giving it a yellowish hue. There is a subtle color gradient, where the outer regions show a marginal increase in bluer light, suggestive of some younger stellar populations toward the outskirts, though the effect is minimal. There is no clear evidence of significant dust lanes or active star formation regions within the galaxy's visible structure based on color. The object exhibits a high Sersic index, which indicates a centrally concentrated profile.
