The galaxy presents as a largely featureless, elliptical structure with a smooth light distribution. The central bulge exhibits a concentrated, bright, yellowish-white core, indicative of an older stellar population. The isophotes appear elongated, with an approximate axis ratio of 0.2, suggesting a relatively flat, cigar-shaped morphology. There's a subtle color gradient noticeable, with the outer regions appearing slightly redder than the core, potentially indicating a difference in stellar population or dust content. No significant signs of tidal disturbances or ongoing major mergers are visible, and the galaxy appears to be relatively isolated. The estimated size is approximately 6 kpc across.
