The galaxy presents as an elliptical morphology, appearing generally smooth with a concentrated central bulge. The light distribution exhibits a radial gradient, peaking in intensity at the core. The overall color is suggestive of an older stellar population with a moderate degree of redness, though bluer components cannot be ruled out due to limitations in resolution. The isophotes exhibit a modest ellipticity. There is no clear evidence of spiral arm structure or significant dust lanes in the available imaging. The galaxy appears undisturbed, with no obvious signs of recent major mergers or tidal interactions.
