The galaxy presents as a relatively smooth, featureless structure with an elliptical morphology. It exhibits a notable central bulge that dominates its overall luminosity. The color profile suggests a greater concentration of older stellar populations, indicated by a redder hue, particularly towards the central region. Fainter, bluer extensions are visible along the major axis, possibly hinting at some ongoing star formation. There appears to be no distinct spiral arm structure or prominent dust lanes visible within the resolution of this image. The galaxy shows a slightly cigar-like shape. There are no indications of ongoing major merging activity, although minor disturbances or interactions cannot be entirely ruled out.
