The galaxy presents as a relatively small, elongated structure, with an apparent smoothness to its overall morphology. There is evidence of a central concentration of light, though without distinct structural features such as spiral arms or a prominent bar. The galaxy appears somewhat cigar-shaped and is not perfectly round. The color profile suggests a redder hue, consistent with an older stellar population and a lower rate of active star formation. No signs of major interactions or significant tidal disturbances are apparent in the immediate vicinity. The galaxy appears to be relatively isolated.
