The galaxy presents a generally smooth morphology, exhibiting a high degree of central concentration. The overall shape appears elliptical, tending towards a moderate ellipticity rather than perfectly spherical. There is no strong evidence of spiral arm structure or a pronounced disk component. Minor disturbances or interactions cannot be ruled out, but a major merger event seems improbable based on the galaxy's overall regularity. The color profile indicates a slightly redder hue, potentially suggesting a stellar population dominated by older, less massive stars, with limited ongoing star formation. There may be a faint nucleus present.
