The galaxy presents an elliptical morphology, exhibiting a smooth, featureless light distribution. There is a noticeable central concentration of luminosity, decreasing gradually outwards from the core. The overall shape is elongated, with a cigar-like appearance rather than a perfectly circular profile. Color gradients are subtle, with a slightly redder hue in the central regions suggestive of an older stellar population. The outer regions appear slightly bluer, possibly indicating the presence of younger stars, though this is not clearly resolved. There's no apparent evidence of spiral arms, dust lanes, or significant tidal disturbances, suggesting a relatively quiescent and evolved system.
