The galaxy presents a generally smooth morphology, appearing largely featureless with a notable absence of defined spiral arms or a prominent central bulge. The light distribution indicates a concentration towards the core, gradually diminishing outwards. The overall shape is elongated, displaying an elliptical form. The dominant color is a yellowish hue, suggesting a population of older stars. There may be ongoing star formation, though it does not appear to be dominant or localized in specific regions. There does not seem to be evidence of recent or ongoing major merger activity or significant tidal disturbances.