The galaxy presents as a single, relatively smooth object with a slightly elongated morphology. It appears centrally condensed, with the light profile gradually decreasing outward. The galaxy exhibits a yellowish-white hue, with a subtle shift towards redder tones in its central regions. There is no clear evidence of spiral arm structure or significant dust lanes. No distinct signs of recent major merger events are observed, although the slight elongation could suggest minor tidal disturbances or interactions in its past. The overall appearance suggests a galaxy dominated by an older stellar population, with relatively low levels of ongoing star formation.
