The galaxy presents a somewhat elongated, cigar-shaped morphology. Its light profile is dominated by a smooth, centrally concentrated component, which appears diffuse. There is evidence of a disturbed structure with the hint of a tidal tail suggesting possible past interactions or mergers. Star formation appears to be relatively low within the galaxy, as indicated by the lack of bright, blue star-forming regions. The color indices suggest a population of older stars, leaning towards the redder end of the spectrum. A single bright spot off to the side suggests active star formation in the surrounding galactic environment. The galaxy appears to be a relatively low-mass object.
