The galaxy presents as a relatively smooth, elliptical-like structure, with a concentrated central bulge exhibiting a yellowish hue, indicative of an older stellar population. Moving outward from the core, the galaxy transitions to a bluish halo, suggesting the presence of younger, hotter stars, although star formation appears subdued overall. The shape is elongated rather than perfectly circular, and shows little or no evidence of spiral arms or significant dust lanes. There is no clear indication of a major merger event, though a slight asymmetry might point to a past minor interaction. The galaxy's overall morphology is suggestive of a system nearing the red sequence, possibly in a transitional stage of star formation activity.
