The galaxy presents as a roughly elliptical shape, appearing elongated with a cigar-like profile. The light distribution is centrally concentrated, showing a smooth morphology. The color profile suggests a dominant older stellar population, as indicated by the reddish-gold hue, likely associated with relatively low levels of ongoing star formation. There is no obvious spiral structure or prominent dust lanes visible. The galaxy seems to be relatively isolated with no signs of major mergers or significant tidal disturbances in this view.
