This galaxy presents an elliptical morphology, with a smooth, featureless appearance. The central bulge is prominent, exhibiting a concentrated luminosity that decreases gradually towards the outer regions. The galaxy appears elongated with a cigar shaped appearance. There is no evidence of significant dust lanes or spiral arm structure. The color profile indicates a concentration of older stellar populations. Light is shifted towards the redder part of the spectrum, consistent with relatively little ongoing star formation. There are no signs of any major disturbance or a merger event.
