The galaxy presents as a concentrated elliptical form, with a centrally bright core. The luminosity appears to gradually diminish with increasing radial distance from the nucleus. The overall color profile tends towards redder hues, which likely indicates an older stellar population with lower ongoing star formation. There appears to be a faint disk structure, but the galaxy is mostly smooth in appearance. The shape of the galaxy is consistent with an elliptical type, exhibiting an elongated shape. The major axis is oriented approximately northwest to southeast. There is evidence of minor disturbances in the galaxy's morphology, potentially suggesting past interactions or mergers.
